The galaxy presents as a well-defined elliptical morphology with a smooth light distribution. The core region is bright and concentrated, exhibiting a yellowish-orange hue indicative of an older stellar population. There is a notable absence of spiral arms or prominent dust lanes. The overall structure appears largely undisturbed, showing no obvious signs of major mergers or tidal distortions, but does show some minor disturbance. The lack of strong blue coloration suggests relatively low ongoing star formation activity. The shape is close to round.
