The galaxy presents as a slightly elongated elliptical morphology, with a smooth and concentrated light distribution. The central region exhibits a bright, yellowish hue indicative of an older stellar population. The outer regions gradually fade into the background sky, displaying a reddish tint. There is no indication of spiral arms or significant dust lanes. The galaxy exhibits a fairly high degree of rotational symmetry. Overall, it appears as a relatively undisturbed, quiescent system.
