The galaxy presents as a centrally concentrated, elliptical morphology. The core region exhibits high surface brightness, appearing almost uniformly luminous. The outer regions fade gradually, with a relatively smooth transition from the bright center to the fainter periphery. The galaxy appears somewhat elongated. There is very little evidence of spiral arm structure or dust lanes within the visible spectrum of this image. Overall, the galaxy displays characteristics consistent with an evolved, early-type galaxy. Faint color variations may be present, potentially indicating subtle differences in stellar populations. The galaxy appears relatively undisturbed.
