The galaxy appears to be a smooth, elliptical galaxy. It exhibits a concentrated central bulge that transitions into a fainter, more diffuse halo. There is a subtle color gradient, with the central bulge displaying a yellowish-orange hue, suggestive of an older stellar population. The outer regions of the galaxy appear slightly bluer, possibly indicating the presence of younger stars or a low level of ongoing star formation. The galaxy is not perfectly spherical, showing a slight elongation. There are no indications of strong tidal features, major mergers, or significant disk structures. Overall, it appears to be a relatively undisturbed, mature galaxy.
