The galaxy presents as a mildly elongated spheroid. The light is predominantly smooth and centrally concentrated, appearing yellowish-white in the central region. The outer regions exhibit a more diffuse, greenish-tinted hue. The overall structure does not show any prominent spiral arms or significant dust lanes. There is a slight deviation from perfect ellipticity, with the shape appearing somewhere between a circular and cigar-shaped distribution. No strong signs of major mergers are visible, though there may be a very minor asymmetry hinting at a past interaction. The smoothness suggests a relatively older stellar population. Based on the light profile, the galaxy seems to be a passively evolving system.
