The galaxy presents as a moderately bright, well-defined elliptical morphology. The light distribution is relatively smooth across the galaxy, with a concentration of intensity towards the central region, indicative of a bulge. There are some disturbances from merging activity. There appears to be a hint of a ring or disk-like feature when looking at it from a profile view. The color profile suggests a population of older stars, especially within the bulge. The smooth light distribution indicates the absence of strong spiral arm structures or prominent dust lanes.
