The galaxy appears to be a relatively smooth, elliptical-type galaxy. It exhibits a centrally concentrated bulge that dominates its overall structure. The light distribution is fairly uniform, without prominent spiral arms or significant dust lanes visible. There is a slight elongation to the galaxy's shape; it is not perfectly spherical, but rather more of a flattened ellipsoid. The galaxy's color is a relatively consistent hue throughout, with a suggestion of a blueish tint, potentially indicating some ongoing, albeit limited, star formation. No strong tidal features or signs of recent major merger activity are immediately apparent, although there are possible indications of a minor disturbance. Overall, the morphology suggests a mature galaxy that has likely undergone significant dynamical relaxation.
