The galaxy presents as a relatively smooth, elliptical-type galaxy. It exhibits a central bulge that appears slightly elongated, with a generally rounded morphology. There is a hint of a disk, with a pale flattened region that surrounds the central bulge. The overall color profile suggests a population of older stars, with a yellow/red hue dominating the central regions, though there is some blue light present. The smooth appearance indicates that the galaxy is likely in a relatively stable state, although there may be some faint disturbances. The galaxy does not obviously present as a merger, although there could be evidence of minor interactions.