| NGC 4825 | |
|---|---|
A PanSTARRS Image of NGC 4825 | |
| Observation data (J2000 epoch) | |
| Constellation | Virgo |
| Right ascension | 12h 57m 12.20s |
| Declination | −13° 39′ 56.00″ |
| Redshift | 0.01475±0.00022 |
| Distance | 230 Mly (70.55 Mpc) |
| Apparent magnitude (V) | 11.9 |
| Characteristics | |
| Type | SA0^- |
| Size | 133,000 ly |
| Apparent size (V) | 2.63′ × 1.585′ |
| Notable features | Turning into spiral(?) |
| Other designations | |
| PGC 44261, LEDA 44261, MCG -02-33-070, GSC 05542-01145 | |
NGC 4825 is a lenticular galaxy located around 230 million light-years away in the constellation Virgo. NGC 4825 was discovered on March 27, 1786 by the astronomer William Herschel, and its diameter is 133,000 light-years across. NGC 4825 is not known to have much star-formation, and it does not have an active galactic nucleus.
NGC 4825 does have one suspected satellite galaxy, J12571108-1339100, a dwarf elliptical galaxy.