This galaxy presents as a relatively smooth, elliptical structure. The light profile increases towards the center, culminating in a bright, moderately concentrated core region. There is a general lack of discernible spiral arms or significant dust lanes within the galaxy's disk. The overall color appears to be a somewhat red, suggesting a population dominated by older stars, and a relatively low ongoing star formation rate. The galaxy's shape is elongated with an axial ratio indicating it is inclined to our line of sight. Minor disturbances are present, suggesting a possibility of a past merger. The overall structure supports the galaxy's classification as an early-type galaxy.
