NGC 4185
NGC 4185 is a large spiral galaxy in the constellation of Coma Berenices. Its velocity with respect to the cosmic microwave background is, which corresponds to a Hubble distance of. Additionally, three non-redshift measurements give a farther mean distance of. It was discovered by German-British astronomer William Herschel on 11 April 1785.
NGC 4195 is a LINER galaxy, i.e. a galaxy whose nucleus has an emission spectrum characterized by broad lines of weakly ionized atoms.