The galaxy presents as a smooth, elliptical-like structure with a concentrated central bulge. The light distribution suggests minimal substructure, such as spiral arms or distinct dust lanes. There is a subtle color gradient, the central region is brighter and appears slightly more yellow-red, transitioning to a bluer hue toward the outer edges. Overall, the galaxy exhibits a diffuse, somewhat spheroidal morphology, indicative of an evolved system. There are no signs of ongoing major mergers or significant tidal disturbances. It looks like the galaxy has finished merging with any close neighbors.
