The galaxy appears as a concentrated spheroid with a smooth light distribution, suggesting an elliptical morphology. The central region exhibits a bright, concentrated luminosity that fades gradually towards the outer edges. The overall color index suggests a population of older stars and little active star formation. There is no visible evidence of spiral arms, bars, or significant dust lanes, which further supports the classification as an elliptical galaxy. The galaxy's symmetric structure shows no clear indication of a major ongoing merger event, although subtle disturbances cannot be ruled out at this resolution. The estimated size appears relatively compact, with the majority of the light concentrated within the central region.
