The galaxy appears to be an elliptical galaxy viewed at an oblique angle. It exhibits a smooth, diffuse light profile without any distinct spiral arm structures or prominent dust lanes. The central region is characterized by a higher surface brightness, suggesting a concentration of stars and potentially a supermassive black hole. The overall color of the galaxy is reddish-yellow, indicative of an older stellar population dominated by red giant stars and a low rate of on-going star formation. The morphology is elongated, with the major axis significantly longer than the minor axis. There is no obvious evidence of a major merger or strong tidal interactions, although some subtle irregularities in the outer regions could suggest minor disturbances.
