NGC 4835 is an intermediate spiral galaxy in the constellation of Centaurus. Its velocity with respect to the cosmic microwave background is 2,441±19 km/s, which corresponds to a Hubble distance of 117.4 ± 8.3 Mly (36.01 ± 2.54 Mpc). However, 18 non-redshift measurements give a much closer mean distance of 75.63 ± 2.73 Mly (23.189 ± 0.836 Mpc). It was discovered by British astronomer John Herschel on 3 June 1834. NGC 4835 has a possible active galactic nucleus, i.e. it has a compact region at the center of a galaxy that emits a significant amount of energy across the electromagnetic spectrum, with characteristics indicating that this luminosity is not produced by the stars.
Galaxy group NGC 4835 is part of a galaxy group known as [CHM2007] LDC 939 which contains four galaxies, including NGC 4976, ESO 219-21, and ESO 269-58.
Supernova One supernova has been observed in NGC 4835:
SN 2025wrd (Type Ia, mag. 17.129) was discovered by ATLAS on 1 September 2025.
See also List of NGC objects (4001–5000)
References
External links NGC 4835 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images


