The galaxy presents as a largely featureless elliptical type. Its morphology is dominated by a smooth, centrally concentrated luminosity profile. The core region exhibits a notably bright and compact nucleus which is surrounded by a diffused halo. There is a subtle color gradient observable, with the core appearing slightly more yellow, suggestive of an older stellar population. The outer regions of the halo transition to a bluer hue indicating the possibility of a more recent, albeit minimal, star formation activity on the outskirts of the galaxy. The overall shape appears to be very close to circular with no evidence of tidal disturbances or ongoing merger events.
