The galaxy presents as a fairly smooth, elliptical-like structure, though the image resolution limits definitive morphological classification. It exhibits a centrally concentrated light profile, with a gradual decrease in brightness outward from the core. The galaxy appears almost perfectly round. The color profile suggests a population dominated by older stars, evidenced by the redder hues that are seen to the right of the galaxy. There is little evidence of distinct spiral arms or significant dust lanes. There is no visually apparent disturbance of the galaxy indicating that it is currently involved in a merger event.
