The galaxy presents as a primarily smooth, elliptical morphology. It exhibits a concentrated central bulge with a gradual decrease in surface brightness towards its outer regions. There is a slight elongation, suggesting a deviation from perfect sphericity. The overall color appears reddish, consistent with an older stellar population. No distinct spiral arms or dust lanes are discernible, and the overall structure indicates minimal ongoing star formation. There is some evidence of minor disturbances in the galaxy's morphology, but it seems to be a relatively isolated system.
