The galaxy presents as a relatively smooth, elliptical or lenticular system. It exhibits a concentrated central bulge with a gradual decrease in surface brightness outwards. The core appears a yellow-white hue, indicating a population of older stars. The outer regions show a slightly bluer tint, suggesting the presence of some younger stars, but the overall color profile indicates a generally quiescent star formation history. There is no evidence of spiral arms or significant dust lanes. The shape is generally in between round and elongated. No signs of major mergers are evident, although a slight asymmetry might indicate a past minor interaction or disturbance.
