This galaxy appears as a centrally concentrated, elliptical-shaped structure, with a smooth, diffuse halo extending outwards. There is a strong central bulge that is notably brighter than the surrounding halo, suggesting a high stellar density in the core. The overall color is consistent with an evolved stellar population. A slight distortion and possible tidal feature can be observed on one side, indicative of a past or ongoing gravitational interaction. There is a slight indication of disk structure, but overall the galaxy appears relatively smooth. The galaxy exhibits signs of an intermediate degree of disturbance, with no major disruptions to its overall form.
