The galaxy presents as a largely featureless elliptical morphology. It exhibits a smooth light profile, with a centrally concentrated luminosity that diminishes gradually towards its outer edges. The core region appears bright, suggestive of a high stellar density. The color profile is relatively uniform across the galaxy, displaying a predominantly yellow-red hue. This coloration suggests a population dominated by older stars, with a low rate of ongoing star formation. There is no visible evidence of spiral arms, a central bar, or significant dust lanes. The overall roundness is relatively high, exhibiting a near circular shape. There are no obvious signs of tidal disturbances or ongoing merger activity.
