The galaxy presents as an elliptical morphology, exhibiting a smooth, largely featureless light distribution. It displays a yellowish-orange hue, indicating a stellar population likely dominated by older, redder stars. The galaxy appears relatively rounded, lacking a pronounced disk structure. There is a possible minor disturbance or interaction evident, with an object appearing very close to it. This interaction does not seem strong enough to classify this galaxy as a merger but could influence its shape.
