The galaxy appears to be a relatively smooth, elliptical-type galaxy, exhibiting a centrally concentrated light profile. There is a clear, bright nucleus, surrounded by a more diffuse halo of light. The galaxy's shape appears to be somewhere between round and slightly elongated. Faint, diffuse features appear near the galaxy, which may indicate tidal interactions or minor disturbances. Color gradients are present, with the central region exhibiting a yellowish hue, potentially indicative of an older stellar population and less active star formation. The outer regions appear slightly bluer, hinting at some younger stars or ongoing, though potentially limited, star formation. The overall morphology suggests a system that is not undergoing a major merger, though minor disturbances cannot be ruled out.
