The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a centrally concentrated luminosity profile, with a bright, yellowish core that gradually fades into a less luminous, diffuse halo. The galaxy appears to be roughly circular in shape, showing no evidence of a strong disk component or significant tidal disturbances. There is a slight color gradient visible, with the central region appearing more yellow, and the outer regions showing a slight bluish tinge. This suggests a population of older stars in the center and a younger stellar population in the outer regions. Overall, the galaxy presents a well-defined, symmetrical structure indicative of a relatively relaxed and evolved system.
