The galaxy appears to be a relatively smooth and centrally concentrated system. It presents an elliptical morphology, with a high degree of central light concentration, suggesting a likely early-type galaxy. The galaxy's overall color is consistent with an older stellar population, potentially indicative of a low star formation rate. There is a subtle hint of a disk-like structure. No major disturbances from ongoing or recent mergers are immediately apparent, though the possibility of minor disturbances can't be excluded without further investigation. The isophotes transition from an elliptical to a slightly more boxy shape with increasing radius. Overall, the galaxy appears relatively undisturbed.