The galaxy presents a centrally concentrated luminosity profile, appearing mostly smooth in morphology, with a notable, yet subtle, disk-like feature. The central region exhibits a bright, compact core. The overall color suggests a population of older stars with a low star formation rate. There's a faint extension visible along one side, which could indicate a tidal interaction or a minor disturbance. The general shape appears somewhat in between round and elongated, with no obvious spiral arm structure. Overall, the galaxy appears to be a relatively undisturbed system.
