The galaxy presents as a somewhat elliptical, centrally concentrated object. It exhibits a smooth, diffuse morphology, suggestive of an early-type galaxy. The central region displays a yellowish hue, potentially indicating an older stellar population. The light profile decreases gradually from the core outwards. There is little evidence of spiral arm structure or significant dust lanes. The overall appearance suggests minimal ongoing star formation activity. There is no obvious evidence of a recent or ongoing merger event although a small asymmetry cannot be ruled out.
