NGC 2325
NGC 2325 is a elliptical galaxy in the constellation of Canis Major. Its velocity with respect to the cosmic microwave background is, which corresponds to a Hubble distance of. However, 16 non-redshift measurements give a much closer mean distance of. It was discovered by British astronomer John Herschel on 1 February 1837.
NGC 2325 is a radio galaxy, i.e. it has giant regions of radio emission extending well beyond its visible structure. It also has an 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.