The galaxy appears to be a relatively smooth, centrally concentrated system. It exhibits a roughly elliptical morphology, being more rounded than elongated. The central region is bright and yellowish-white, suggesting an older stellar population. A bluer, more diffuse halo surrounds the core, indicating the presence of some younger stars and potentially ongoing, but low-level, star formation. There is a slight asymmetry to the outskirts of the galaxy, with a possible minor disturbance or tidal feature visible on one side. This could be indicative of a past or ongoing minor merger event. The overall color is intermediate, suggesting a mix of stellar populations, and a mass within the range typical for galaxies of this type.
