The galaxy presents as a moderately bright, elliptical or lenticular-shaped structure. A central bulge is readily apparent, displaying high luminosity and a smooth, concentrated distribution of light. The luminosity decreases outwards from the bulge. 

There is evidence of a faint disk component that appears slightly disturbed or warped, as well as possible tidal features. These features consist of faint asymmetric extensions of light suggesting gravitational interactions. The shape of the outer regions is somewhere in between round and elliptical, and does not show a clear spiral structure. There are some indications of ongoing or recent merger activity.
