The galaxy presents an elliptical morphology, appearing largely smooth and lacking discernible spiral arm structures. The primary color appears to be a yellowish-white, potentially indicative of an older stellar population. There is a slight elongation visible in the galaxy's shape, giving it a cigar-like appearance. This elongation is not suggestive of a disk, but rather an ellipsoidal distribution of stars. No significant dust lanes or prominent star-forming regions are clearly observed. The lack of distinct features and the smoothness of the light distribution point towards a system dominated by relatively evolved stars and a low current star formation rate. There is no strong evidence of a recent or ongoing major merger event.
