The galaxy presents as a generally smooth and centrally concentrated object. It exhibits a spheroidal morphology, appearing largely elliptical with little discernible disk structure or spiral arms. The galaxy has a bright, yellowish core that gradually fades into a less luminous halo. The color suggests an older stellar population with lower levels of recent star formation. There are indications of some minor disturbances in the overall shape, possibly hinting at past interactions or mergers, although these are not pronounced. The object appears relatively isolated, with no immediately apparent signs of ongoing major merging activity.
