The galaxy appears as a lenticular-type object, exhibiting both smooth and disk-like characteristics. It presents an elliptical, elongated morphology. There is an apparent central bulge of concentrated luminosity. There are what appears to be some tidal disturbances or perhaps a sign of a recent or on-going merger event, or maybe some irregular features, which are more prominent on one side of the galaxy than the other. There are two distinct features on the left side of the galaxy, with one feature brighter than the other. The object is dominated by older stellar populations, with hints of active star formation, but appears to have an aging stellar population.
