| NGC 7645 | |
|---|---|
NGC 7645 imaged by Legacy Surveys | |
| Observation data (J2000 epoch) | |
| Constellation | Sculptor |
| Right ascension | 23h 23m 47.3070s |
| Declination | −29° 23′ 17.083″ |
| Redshift | 0.023086±0.00000900 |
| Heliocentric radial velocity | 6,921±3 km/s |
| Distance | 318.6 ± 22.3 Mly (97.68 ± 6.84 Mpc) |
| Apparent magnitude (V) | 13.77 |
| Characteristics | |
| Type | SB(r)c |
| Size | ~205,600 ly (63.04 kpc) (estimated) |
| Apparent size (V) | 1.4′ × 1.2′ |
| Other designations | |
| ESO 470- G 003, 2MASX J23234727-2923170, MCG -05-55-007, PGC 71314 | |
NGC 7645 is a barred spiral galaxy in the constellation of Sculptor. Its velocity with respect to the cosmic microwave background is 6,623±21 km/s, which corresponds to a Hubble distance of 318.6 ± 22.3 Mly (97.68 ± 6.84 Mpc). It was discovered by British astronomer John Herschel on 27 September 1834.

According to Soares and colleagues, NGC 7645 and NGC 7636 form a galaxy pair with a probability of 0.57. The Hubble distance to NGC 7636 is 323.1 ± 22.7 Mly (99.06 ± 6.96 Mpc), which is close to that of NGC 7645. The galaxies are separated by an angular distance of 17.4′.
Two supernovae have been observed in NGC 7645: