This galaxy presents as a relatively smooth, elliptical-like structure. The light distribution appears centrally concentrated, with a gradual decrease in surface brightness outwards from the core. No prominent spiral arms or bar features are discernible. There are no features that would suggest a major disturbance, strong asymmetry, or interaction. The color profile suggests a population dominated by older stars, with a reddish hue implying relatively low recent star formation activity. The overall impression is that of a mature system, potentially with ongoing but limited star formation. The shape seems to be that of an in-between round galaxy.
