The galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a concentrated luminosity, appearing yellowish-white in color, suggestive of an older stellar population. Moving outward from the core, a gradual decrease in surface brightness is observed. A bluer halo surrounds the central bulge. No distinct spiral arms or dust lanes are discernible. There is a slight indication of tidal features. The galaxy appears to be experiencing limited star formation activity. Overall, the galaxy presents as a somewhat disturbed system without any major mergers.
