The galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated central bulge that transitions smoothly to a more diffuse halo. There is a slight color gradient, with the core of the galaxy appearing more yellow/orange. This might be due to the high concentration of older stars. There are some indications of possible tidal disturbances, but they are faint. Based on the color and general morphology, this galaxy is likely composed of older stars with little active star formation. The galaxy is relatively isolated, with no obvious major interacting companions, but there could be a recent or ongoing merger. The smooth appearance and round morphology indicate this galaxy has experienced major mergers in the past, creating its smooth, relaxed structure.
