The galaxy appears to be an elliptical galaxy, or potentially a lenticular galaxy with a very faint disk component. It presents a smooth, largely featureless morphology, with a high degree of central concentration. The light profile is generally ellipsoidal and fairly well-rounded in appearance. There is a gradual decrease in surface brightness moving outwards from the nucleus.

The galaxy exhibits a color gradient, with the central region appearing more yellowish-white, possibly indicative of a population of older stars. The outer regions have a slightly bluer tint, suggesting the presence of a younger stellar population, or perhaps some level of recent star formation. There are no obvious tidal features, nor evidence of ongoing major mergers. However, very subtle irregularities, or evidence of a minor interaction in the recent past, cannot be entirely ruled out.
