| UGC 4904 | |
|---|---|
UGC 4904, imaged by the Sloan Digital Sky Survey | |
| Observation data (J2000 epoch) | |
| Constellation | Lynx |
| Right ascension | 09h 17m 22.062s |
| Declination | +41° 54′ 39.70″ |
| Redshift | 0.005571 |
| Heliocentric radial velocity | 1665 |
| Distance | 90.5 ± 6.4 Mly (27.74 ± 1.96 Mpc) |
| Apparent magnitude (B) | 15.0 |
| Characteristics | |
| Type | SABdm |
| Size | ~31,200 ly (9.58 kpc) (estimated) |
| Notable features | Dwarf spiral galaxy with a supernova impostor which eventually exploded as an actual supernova |
| Other designations | |
| MCG +07-19-054, PGC 26231, CGCG 209-044 | |
UGC 4904 is a barred spiral galaxy in the constellation Lynx. Its velocity with respect to the cosmic microwave background is 1880 ± 15 km/s, which corresponds to a Hubble distance of 90.5 ± 6.4 Mly (27.74 ± 1.96 Mpc). The first known reference to this galaxy comes from Part 2 of the Morphological Catalogue of Galaxies, published in 1964, where it is listed as MCG +07-19-054.

On October 20, 2004, a supernova impostor was observed by Japanese amateur astronomer Kōichi Itagaki within the galaxy. This same star may have transitioned from a luminous blue variable star to a Wolf–Rayet star shortly before it was observed as blowing up as supernova SN 2006jc (Type Ibn, mag. 13.8) on October 11, 2006.