The galaxy appears to be a relatively smooth, elliptical or lenticular type. It is centrally concentrated with a diffuse halo extending outwards. There is a slight bluing in the central region, suggesting some ongoing star formation, although the overall color is more consistent with an older stellar population. A minor asymmetry can be seen in the outer regions, possibly caused by a weak interaction with a nearby galaxy, or perhaps due to the presence of a faint tidal tail. The galaxy is moderately luminous, but is not particularly massive.
