The galaxy presents as an elliptical morphology, potentially an E4 or E5 on the Hubble scale. Its light profile is dominated by a smooth, centrally concentrated bulge component. The color index suggests a relatively old stellar population, with the presence of some recent star formation in a disk component. There are noticeable dust lanes or regions of obscuration present.

The galaxy's shape indicates it may be undergoing tidal interactions or a minor merger event. There appears to be some asymmetry, as well as a slight disruption in the light profile. This disturbance is consistent with a system that has experienced past merger activity and is in the process of reaching dynamical equilibrium.
