The galaxy presents as a centrally concentrated, elliptical-like object with a smooth overall appearance. Its core exhibits a yellowish-white hue, suggestive of an older stellar population. The galaxy's light profile appears to gradually fade from the bright center towards the outer edges, with the outermost regions displaying a reddish tint. The apparent elongated shape might indicate a deviation from perfect sphericity. There are subtle indications of a disk. There is a hint of disturbance in the form of a slightly irregular structure or asymmetry. This might indicate that the galaxy is undergoing, or has recently undergone, a minor interaction or merger.