Historical Identification: Per Dreyer, NGC 7300 (= GC 4801 = GC 4799 = JH 2164, 1860 RA 22 23 28, NPD 104 43.5) is "very faint, considerably small, extended, very gradually a little brighter middle." The second IC notes "7300 is not considerably small, but pretty large, extended 150 degrees (John Herschel and Herbert Howe)".
Physical Information: Apparent size 1.9 by 0.75 arcmin (from the images below).

Historical Identification: Per Dreyer, NGC 7301 (Leavenworth list I (#252), 1860 RA 22 24 20, NPD 108 18.2) is "very faint, pretty small, a little extended, a little brighter middle."
Physical Information: Apparent size about 0.8 by 0.45 arcmin (from the images below).

Historical Identification: Per Dreyer, NGC 7302 (= GC 4802 = JH 2165 = WH IV 31, 1860 RA 22 24 54, NPD 104 50.4) is "faint, pretty small, round, very suddenly brighter middle and small nucleus."
Physical Information: Apparent size of about 1.65 by 0.95 arcmin (from the images below).

Historical Identification: Per Dreyer, NGC 7303 (= GC 4804 = JH 2166, 1860 RA 22 25 00, NPD 59 46.4) is "very faint, small, round, gradually a very little brighter middle." The second IC adds "Bigourdan 452 is 2 seconds preceding (to the west of) this. I assume it is a very faint double star that I saw in 1875 100 arcsec south-preceding-preceding (west southwes)t, as Bigourdan says his object may be a cluster".
NOTE TO SELF: The pair of stars referred to by Dreyer is 7.5 seconds of time to the west, so whether it is Big452 is not certain.
Physical Information: Apparent size about 1.7 by 1.3 arcmin (from the images below).

Historical Identification: Per Dreyer, NGC 7304 (= GC 4803, d'Arrest, 1860 RA 22 25 02, NPD 59 45.3) is "very faint, pretty small, a very little brighter middle, north-following (northeast of) h 2166 (?)," (JH) 2166 being NGC 7303. The position precesses to RA 22 31 29.2, Dec +30 57 46, but that lies about 0.9 arcmin to the west-northwest of NGC 7303, so that cannot be the correct position for d'Arrest's object. To determine the correct position, we can compare d'Arrest's observations of JH 2166 to those for his "nova" (made on the same night); doing so shows that he put his nova 2 seconds of time to the east and 1.2 arcmin of declination to the north of NGC 7303 (precessing from his 1861 positions to J2000 positions does not change the result). Given the modern position of NGC 7303, that yields a position for d'Arrest's nova of RA 22 31 34.8, Dec +30 58 34 (whence the position shown above), which lies slightly to the northeast of NGC 7303, but there is nothing there that d'Arrest could have seen. Neither d'Arrest, looking for it on another night, nor Bigourdan or Dreyer (using the largest telescope in the world, Lord Rosse's 72-inch "Leviathan") could find anything that could be NGC 7304, and it is certain that the object simply does not exist.
Observational Notes: Bigourdan actually looked for this on three occasions, once after d'Arrest published his work but before the NGC was published, and twice after the NGC was published. On all three occasions he wrote that he couldn't find anything, or that he couldn't find anything except NGC 7303. Dreyer's failure to observe the object is undoubtedly why he put a question mark at the end of the NGC entry.
Historical Misidentifications: Some references (e.g., HyperLEDA) list a triplet of stars near RA 22 31 44.4, Dec +30 58 47 as NGC 7304, but they cannot be what d'Arrest thought he saw, as his measurements are too accurate to be that far "off", and if that triplet had been what he saw, he almost certainly would have seen it on his second attempt. So they are only mentioned here as a warning about that erroneous identification. The UGC also misidentifies NGC 7304, but as a duplicate of NGC 7303, which it most certainly is not.

Historical Identification: Per Dreyer, NGC 7305 (Swift list IV (#84), 1860 RA 22 25 16, NPD 79 00.3) is "extremely faint, small, round, 4 faint stars around."
Physical Information: Apparent size of about 1.0 by 1.0 arcmin (from the images below).

Historical Identification: Per Dreyer, NGC 7306 (= GC 4805 = JH 3948, 1860 RA 22 25 28, NPD 117 58.1) is "very faint, small, a little extended, 11th magnitude star preceding (to west)."
Physical Information: Apparent size of about 1.45 by 0.7 arcmin (from the image below).

Historical Identification: Per Dreyer, NGC 7307 (= GC 4806 = JH 3947, 1860 RA 22 25 33, NPD 131 39.9) is "faint, pretty large, pretty much extended."
Physical Information: NGC 7307 is listed as a member of a group of galaxies in or near Sculptor with recessional velocities of about 1500 to 1800 km/sec (this is not "the" Sculptor Group, a close neighbor to our Local Group, with an average recessional velocity of less than 300 km/sec). Apparent size of about 3.9 by 1.05 arcmin (from the images below).

Historical Identification: Per Dreyer, NGC 7308 (Leavenworth list I (#253), 1860 RA 22 26 25, NPD 103 42.2) is "pretty bright, very small, round." The second IC lists a corrected RA (per Howe) of 22 27 05.
Physical Information: Apparent size of about 1.1 by 0.8 arcmin (from the images below).

Historical Identification: Per Dreyer, NGC 7309 (= GC 4807 = JH 2167 = WH II 476, 1860 RA 22 26 56, NPD 101 04.9) is "very faint, pretty large, round, gradually a little brighter middle, mottled but not resolved." (Dreyer's NGC entry is misprinted as 7319).
Physical Information: Apparent size of about 1.9 by 1.6 arcmin (from the images below).

Historical Identification: Per Dreyer, NGC 7310 (Leavenworth list I (#254), 1860 RA 22 27, NPD 113 14.3) is "very faint, pretty small, round, brighter middle and nucleus." The second IC lists a corrected RA (per Howe) of 22 26 57.
Physical Information: Apparent size of about 0.9 by 0.7 arcmin (from the images below).

Historical Identification: Per Dreyer, NGC 7311 (= GC 4808 = JH 2168 = WH II 428, 1860 RA 22 27 03, NPD 85 09.0) is "pretty faint, small, round, pretty suddenly brighter middle, mottled but not resolved."
Physical Information: Based on a recessional velocity of 4535 km/sec, NGC 7311 is about 210 million light years away, in good agreement with redshift-independent distance estimates of 180 to 220 million light years. Given that and its apparent size of about 1.6 by 0.75 arcmin (from the images below), it is about 100 thousand light years across.

Historical Identification: Per Dreyer, NGC 7312 (= GC 6058, Marth #485, 1860 RA 22 27 32, NPD 84 54) is "faint, small."
Physical Information: Apparent size of about 1.15 by 0.9 arcmin (from the images below).

Historical Identification: Per Dreyer, NGC 7313 (= GC 6059, Marth #486, 1860 RA 22 27 46, NPD 116 50) is "extremely faint, extended."
Physical Information: Apparent size of about 0.5 by 0.35 arcmin (from the images below).

Historical Identification: Per Dreyer, NGC 7314 (= GC 4810 = JH 3949, 1860 RA 22 28 02, NPD 116 45.9) is "considerably faint, large, much extended 0°, a very little brighter middle." The position precesses to RA 22 35 47.1, Dec -26 02 32, within the northeastern outline of the galaxy listed above, the description fits and there is nothing else nearby, so the identification is certain.
Physical Information: NGC 7314 is a Seyfert galaxy (type S1h). Based on a recessional velocity of 1430 km/sec (and H₀ = 70 km/sec/Mpc), it is about 65 million light years away, in good agreement with redshift-independent distance estimates of 50 to 70 million light years. Given that and its apparent size of about 4.6 by 1.9 arcmin (from the images below), it is nearly 90 thousand light years across. NGC 7314 is listed as a member of a group of galaxies in or near Sculptor with recessional velocities of about 1500 to 1800 km/sec (this is not "the" Sculptor Group, a close neighbor to our Local Group, with an average recessional velocity of less than 300 km/sec).
Arp Atlas Designation: NGC 7314 is used in the Arp Atlas of Peculiar Galaxies as an example of a spiral galaxy with detached segments, correctly identified as NGC 7314, and with the note "Almost no nucleus".

Historical Identification: Per Dreyer, NGC 7315 (= GC 6060, Stephan list IV (#13), 1860 RA 22 29 08, NPD 55 55.0) is "very faint, extremely small, round, brighter middle."
Physical Information: Apparent size of about 1.5 by 1.5 arcmin (from the images below).

Historical Identification: Per Dreyer, NGC 7316 (= GC 3809 = JH 2169 = WH III 180, d'Arrest, 1860 RA 22 29 11, NPD 70 24.1) is "faint, small, round, 8th magnitude star south-preceding (to southwest)."
Physical Information: Apparent size of about 1.05 by 0.9 arcmin (from the images below).

Historical Identification: Per Dreyer, NGC 7317 (= GC 6061, Stephan list VIII (#19), 1860 RA 22 29 30, NPD 56 46.7) is "very faint, very small."
Physical Information: NGC 7317 is one of the four galaxies in Stephan's Quintet that are at about the same distance from us (NGC 7320 is merely a foreground galaxy). Based on its recessional velocity of 6600 km/sec, NGC 7317 is about 310 million light years away. Given that and its apparent size of 0.7 by 0.7? arcmin, it is about 65 thousand light years across.

Historical Identification: Per Dreyer, NGC 7318 (= GC 6062, Stephan list VIII (#20), 1860 RA 22 29 35, NPD 56 45.5) is "extremely faint, extremely small."
Physical Information: NGC 7318 represents two of the four galaxies in Stephan's Quintet that are at about the same distance from us (NGC 7320 is merely a foreground galaxy). Based on a recessional velocity of 6630 km/sec, PGC 69260 (the western member of the pair) should be about 310 million light years away, which is about the same distance as NGC 7317. However, there must be a substantial effect due to peculiar (non-Hubble-expansion) velocities, since PGC 69263, which is strongly interacting with PGC 69260 and must be at the same distance, has a recessional velocity of only 5775 km/sec, which corresponds to a distance of only 270 million light years. That value is probably too low, and the other distance probably too high, and the pair must have an actual distance around 290 million light years (give or take at least 10 million light years). Given that, PGC 69260's apparent size of 1.3 by 1.2 arcmin corresponds to about 110 thousand light years, and PGC 69263's apparent size of 2.0 by 1.0 arcmin corresponds to about 170 thousand light years (these sizes probably include the clouds of gas and stars ejected from the main structures by their gravitational interaction).

Below, a ? arcmin wide infrared image of the region shows (in false-color green) a region of gas larger than our Milky Way galaxy colliding with the esatern side of NGC 7318 at more than a million miles an hour. The shock wave caused by that collision heats up the gas (causing the radiation shown in the image) and compresses it, forming knots of hot, bright young stars seen scattered throughout the region in the visible-light images above. (Infrared Image Credit NASA/JPL-Caltech/Max-Planck Institute/P. Appleton (Spitzer Science Center / Caltech), Spitzer Space Telescope)

Historical Identification: Per Dreyer, NGC 7319 (= GC 6063, Stephan list VIII (#21), 1860 RA 22 29 40, NPD 56 44.8) is "extremely faint, extremely small."
Physical Information: NGC 7319 is one of the four galaxies in Stephan's Quintet that are at about the same distance from us (NGC 7320 is merely a foreground galaxy). Based on a recessional velocity of 6745 km/sec, NGC 7319 is about 300 million light years away, which is about the same as the estimated distances for the other members of the group. Given that and its apparent size of 1.7 by 1.3 arcmin, it about 150 thousand light years across, and a long arm of ejected material extends another 200 thousand light years or so to its southwest. Presumably due to its gravitational interaction with the other members of the Quintet, NGC 7319 is a Seyfert galaxy (type Sy 2).

Historical Identification: Per Dreyer, NGC 7320 (= GC 6064, Stephan list VIII (#22), 1860 RA 22 29 41, NPD 56 46.5) is "faint, very small."
Physical Information: Although listed as a member of Stephan's Quintet (because discovered by Stephan at the same time, and in the same direction), NGC 7320 is unconnected to the other galaxies in the group, being nearly ten times closer to us. Based on a recessional velocity of 785 km/sec, NGC 7320 is about 35 million light years away. However, for such small distances, peculiar (non-Hubble-expansion) velocities can significantly affect the distance estimate, and the value is considerably less than redshift-independent estimates of 45 to 60 million light years; so for the purposes of this discussion, I have assumed an approximate distance of about 50 million light years. Given that and its apparent size of 2.2 by 1.1 arcmin, the galaxy is probably about 30 thousand light years across.

Note About Non-Standard Designations: The use of NGC/IC designations plus letters is common but inconsistent, and has led to errors in assigning physical data to one galaxy or another; hence my usual use of the PGC (Principal Galaxy Catalog) designation as shown above. However, the original PGC only had about 73,000 entries, and although LEDA lists several million supplementary entries (which are used throughout this catalog), their use is "deprecated", meaning discouraged whenever better designations are available. In this case, the preferred designation would be 2MASXJ22363213+3347456, as also shown above.
Physical Information: PGC 3965656 has no apparent relationship to NGC 7320, so save for being within a quarter degree of Stephan's Quintet, it is a mystery why it received its faux NGC name. Other than its apparent size (about 0.7 by 0.15 arcmin from the images below), there appears to be nothing available.

Physical Information: Based on a recessional velocity of 6380 km/sec, PGC 69346 is about 300 million light years away. Given that and its apparent size of about 0.8 by 0.2 arcmin (from the images below), it is about 75 thousand light years across.

Physical Information: Based on a recessional velocity of 5985 km/sec, PGC 69279 is about 280 million light years away, which is close to the average distance of Stephen's Quintet, so unlike NGC 7320, which is a foreground galaxy, PGC 69279 may be a member of the main group. Given that distance and its apparent size of 0.7 by 0.45 arcmin (from the images below), it is about 55 thousand light years across.

Historical Identification: Per Dreyer, NGC 7321 (= GC 4811 = JH 2170 = WH III 237, 1860 RA 22 29 45, NPD 69 06.1) is "faint, small, irregularly round, very gradually a very little brighter middle."
Physical Information: Apparent size of about 1.5 by 1.1 arcmin (from the images below).

Historical Identification: Per Dreyer, NGC 7322 (= GC 4812 = JH 3950, 1860 RA 22 29 46, NPD 127 57.2) is "very faint, small, very little extended, gradually brighter middle."
Physical Information: Apparent size of about 0.9 by 0.55 arcmin (from the images below).

Historical Identification: Per Dreyer, NGC 7323 (= GC 6065, Marth #487, 1860 RA 22 30 06, NPD 71 35) is "pretty faint, pretty large, irregularly round."
Physical Information: Apparent size of about 1.3 by 1.0 arcmin (from the images below).

Historical Identification: Per Dreyer, NGC 7324 (= GC 6066, Marth #488, 1860 RA 22 30 14, NPD 71 34) is "very faint, very small, nebulous star."
Physical Information: Apparent size of about 0.85 by 0.5 arcmin (from the images below).

Historical Identification: Per Dreyer, NGC 7325 (= GC 6067, Schultz (#10, Nova VIII), 1860 RA 22 30 25, NPD 56 21.4) is "faint, very small, h 2172 following (to east)." (JH) 2172 being NGC 7331.

Historical Identification: Per Dreyer, NGC 7326 (= GC 6068, 4th Lord Rosse, 1860 RA 22 30 27, NPD 56 18.2) is "considerably faint, extremely small, h 2172 following (to east)," (JH) 2172 being NGC 7331.

Historical Identification: Per Dreyer, NGC 7327 (Temple list V, 1860 RA 22 30 30, NPD 56 15) is "extremely faint, extremely small, north-preceding (northwest of) h 2172," (JH) 2172 being NGC 7331.
Warning About Misidentification: Steinicke lists NGC 7327 as the star listed above, but that is east of NGC 7331, while Tempel stated his nova was northwest of that galaxy, so Steinicke's identification must be wrong; but some references are bound to use the incorrect identification (as did this entry until I referred to Dreyer's and Corwin's notes on the subject). Unfortunately, just which object northwest of NGC 7331 is NGC 7327 is not obvious, so for now this entry merely points out that the previous identification was incorrect, and a discussion of the more likely "correct" identifications must wait for the next iteration of this page.

Historical Identification: Per Dreyer, NGC 7328 (= GC 4813 = JH 2171, 1860 RA 22 30 31, NPD 80 11.7) is "extremely faint, pretty small, a little extended 90°, very gradually a little brighter middle."
Physical Information: Apparent size of about 2.05 by 0.7 arcmin (from the images below).

Historical Identification: Per Dreyer, NGC 7329 (= GC 4814 = JH 3951, 1860 RA 22 30 37, NPD 157 12.3) is "pretty bright, pretty small, much extended 90°." The position precesses to RA 22 40 24.9, Dec -66 28 40, essentially dead center on the galaxy listed above, the description fits and there is nothing else nearby, so the identification is certain.
Physical Information: Based on a recessional velocity relative to the Cosmic Microwave Background radiation of 3150 km/sec (and H₀ = 70 km/sec/Mpc), NGC 7329 is about 145 to 150 million light-years away, in good agreement with redshift-independent distance estimates of about 70 to 175 million light-years. Given that and its apparent size of about 4.2 by 2.7 arcmin (from the images below), the galaxy is about 180 thousand light-years across.

Historical Identification: Per Dreyer, NGC 7330 (= GC 6069, Stephan list II (#30), 1860 RA 22 30 40, NPD 52 10.6) is "pretty bright, small, a little extended, brighter middle."
Physical Information: Apparent size of about 1.5 by 1.2 arcmin (from the images below).

Historical Identification: Per Dreyer, NGC 7331 (= GC 4815 = JH 2172 = WH I 53, 1860 RA 22 30 40, NPD 56 18.5) is "bright, pretty large, pretty much extended 163°, suddenly much brighter middle."
Physical Information: Apparent size 10.2 by 4.2? arcmin. As noted in the press release for the HST image at the bottom, in many respects, NGC 7331 is just like our Milky Way galaxy. It has a similar size, similar numbers and types of stars, and a similar spiral structure. However, it does not have the central bar that our galaxy is now known to have, and the stars in its core are rotating around the center of the galaxy in the opposite direction from the stars in the spiral arms and disk.
 Note: Although some images of NGC 7331 are shown below, several others will be posted when a discussion of the galaxy's physical characteristics is added to this entry (presumably in the next iteration of this page).

Historical Identification: Per Dreyer, NGC 7332 (= GC 4821 = JH 2173 = WH II 233, 1860 RA 22 30 44, NPD 66 55.6) is "considerably bright, small, much extended 156°, suddenly much brighter middle and nucleus, preceding (western) of 2," the other being NGC 7339.
Physical Information: Apparent size of about 3.3 by 0.65 arcmin (from the images below).

Historical Identification: Per Dreyer, NGC 7333 (= GC 6070, Schultz (#9, Nova IX), 1860 RA 22 30 48, NPD 56 17.3) is "very faint, very small, preceding (west of) h 2174", (JH) 2174 being NGC 7335.
Observational Note: In the NGC notes Dreyer states "Not noticed at Birr nor by Tempel, nor does it occur in an Armagh observation of 1886." This is understandable, since all the observers involved would have been looking for a nebulous object, so this double star wouldn't have drawn any attention.

Historical Identification: Per Dreyer, NGC 7334 (= GC 4822 = JH 3950?, 1860 RA 22 30 50, NPD 127 55.8) is "most extremely faint (= GC 4812?)," the parenthetic question indicating that Dreyer thought this might be the same as GC 4812 (= NGC 7322), which it is.
Physical Information: Given the duplicate entry, see NGC 7322 for anything else.

Historical Identification: Per Dreyer, NGC 7335 (= GC 4823 = JH 2174 = WH III 166, 1860 RA 22 30 56, NPD 56 16.7) is "very faint, very small (B of 3rd Lord Rosse)", the parenthetic comment indicating that this was labeled B in a sketch of the region observed by the 3rd Lord Rosse and his assistant, George Stoney.
Discovery Notes: Lord Rosse and his assistant both examined the region near NGC 7331 in detail on Sep 10, 1849. Two nights later Stoney measured the position of the "knots" near that galaxy, which were labeled with various letters in their notes and in sketches of the region. Whether Rosse was present when Stoney measured the positions isn't clear, but he was present when they were first observed, so both of them are credited in the four entries involved (NGC 7335, 7336, 7337 and 7340).
Physical Information: Apparent size of about 1.15 by 0.6 arcmin (from the images below).

Historical Identification: Per Dreyer, NGC 7336 (= GC 4816, 3rd Lord Rosse, 1860 RA 22 30 59, NPD 56 14.8) is "extremely faint, very small (C)," the parenthetic note indicating that this was labeled C in a sketch of the region observed by the 3rd Lord Rosse and his assistant, George Stoney.
Discovery Notes: Although Dreyer credits the discovery to William Parsons, 3rd Earl of Rosse, he notes that many of Rosse's nebular discoveries were actually made by one of his assistants, in this case George Stoney; but Lord Rosse was also present on the night in question, and also observed the object, as noted above.
Physical Information: Apparent size of about 0.65 by 0.3 arcmin (from the images below).

Historical Identification: Per Dreyer, NGC 7337 (= GC 4817, 3rd Lord Rosse, 1860 RA 22 31 03, NPD 56 21.2) is "extremely faint, small, stellar (E)," the parenthetic comment indicating that this was labeled E in a sketch of the region observed by the 3rd Lord Rosse and his assistant, George Stoney.
Discovery Notes: Although Dreyer credits the discovery to William Parsons, 3rd Earl of Rosse, he notes that many of Rosse's nebular discoveries were actually made by one of his assistants, in this case George Stoney; but Lord Rosse was also present on the night in question, and also observed the object, as noted above.
Physical Information: Apparent size of about 1.3 by 1.2 arcmin (from the images below).

Historical Identification: Per Dreyer, NGC 7338 (Tempel list V, 1860 RA 22 31 03, NPD 56 18) is "extremely faint, extremely small, south-following (southeast of) h 2174," (JH) 2174 being NGC 7335.
Warning About Misidentification: Steinicke lists NGC 7338 as a star at RA 22 36 46.8, Dec +34 27 47, but that is west of NGC 7331, while Tempel stated his nova was southeast of NGC 7335, so Steinicke's identification must be wrong; but some references are bound to use the incorrect identification (as did this entry until I referred to Dreyer's and Corwin's notes on the subject).

Historical Identification: Per Dreyer, NGC 7339 (= GC 4824 = JH 2175 = WH II 234, 1860 RA 22 31 06, NPD 66 56.4) is "faint, pretty small, much extended 89°, very gradually a little brighter middle, following (eastern) of 2," the other being NGC 7332.
Physical Information: Apparent size of about 2.8 by 0.7 arcmin (from the images below). Since the galaxy is seen edge-on, classification is difficult.

Historical Identification: Per Dreyer, NGC 7340 (= GC 4818, 3rd Lord Rosse, 1860 RA 22 31 20, NPD 56 19.0) is "very faint, very small, (D of 3rd Lord Rosse)," the parentheic comment indicating that this was labeled D in a sketch of the region observed by the 3rd Lord Rosse and his assistant, George Stoney.
Discovery Notes: Although Dreyer credits the discovery to William Parsons, 3rd Earl of Rosse, he notes that many of Rosse's nebular discoveries were actually made by one of his assistants, in this case George Stoney; but Lord Rosse was also present on the night in question, and also observed the object, as noted above.
Physical Information: Apparent size of about 1.0 by 0.7 arcmin (from the images below).

Historical Identification: Per Dreyer, NGC 7341 (Leavenworth list I (#255), 1860 RA 22 31, NPD 113 25.3) is "pretty faint, pretty small, extended, a little brighter middle." The first IC lists a corrected RA (per Ormond Stone) of 22 31 27.
Physical Information: Apparent size of about 2.2 by 0.9 arcmin (from the images below). Its unusually bright nucleus suggests it may be a Seyfert galaxy.

Historical Identification: Per Dreyer, NGC 7342 (= GC 6071, Stephan list IV (#14), 1860 RA 22 31 51, NPD 55 13.7) is "extremely faint, very small."
Physical Information: Apparent size of about 1.3 by 1.2 arcmin (from the images below).

Historical Identification: Per Dreyer, NGC 7343 (= GC 6072, Stephan list VIII (#23), (Safford 53), 1860 RA 22 32 13, NPD 56 39.4) is "extremely faint, very small, round, a little brighter middle, small (faint) star involved."
Discovery Notes: Safford's observations were not published until long after the fact, so Dreyer didn't become aware of them until he was in the last stages of preparing the publication of the NGC. As a result they were only mentioned in an appendix, and none of the individual NGC entries gave Safford credit for his observations (hence the inclusion of his name in parentheses).
Physical Information: Apparent size of about 0.95 by 0.7 arcmin (from the images below).

Historical Identification: Per Dreyer, NGC 7344 (= GC 6073, Marth #489, 1860 RA 22 32 21, NPD 94 53) is "pretty faint, very small, round."
Physical Information: Apparent size of about 1.3 by 0.65 arcmin (from the images below).

Historical Identification: Per Dreyer, NGC 7345 (= GC 6074, Stephan list IV (#15), 1860 RA 22 32 22, NPD 55 11.2) is "extremely faint, very small."
Physical Information: Apparent size of about 1.3 by 0.2 arcmin (from the images below). The nucleus has a slightly X-shaped contour, which I have seen in similarly edge-on images of a few other lenticular galaxies.

Historical Identification: Per Dreyer, NGC 7346 (= GC 6075, Marth #490, 1860 RA 22 32 39, NPD 79 39) is "extremely faint, very small, stellar."
Physical Information: Apparent size of about 0.6 by 0.45 arcmin (from the images below).

Historical Identification: Per Dreyer, NGC 7347 (= GC 4825 = JH 2176, 1860 RA 22 32 58, NPD 79 42.7) is "extremely faint, pretty large, extended."
Physical Information: Apparent size of about 1.6 by 0.3 arcmin (from the images below).

Historical Identification: Per Dreyer, NGC 7348 (= GC 6076, Marth #491, 1860 RA 22 33 39, NPD 78 50) is "very faint, pretty large, irregularly round."
Physical Information: Apparent size of about 1.15 by 0.6 arcmin (from the images below).

Historical Identification: Per Dreyer, NGC 7349 (Muller list II (#469), 1860 RA 22 33 52, NPD 113 37.3) is "extremely faint, very small, extended 175°, binuclear, brighter on north side."
Physical Information: Apparent size Based on a recessional velocity of 4480 km/sec, NGC 7349 is about 210 million light years away, about 35 million light years beyond redshift-independent distance estimates of about 175 million light years. Presuming an intermediate distance of about 200 million light years, its apparent size of about 1.0 by 0.3 arcmin (from the images below) corresponds to about 60 thousand light years.