The galaxy presents a largely smooth, elliptical morphology. The core region is dominated by a bright, concentrated luminosity, appearing almost spherical. Moving outward, the galaxy exhibits a gradual decline in surface brightness, transitioning into a less defined, more diffuse halo. There is a very faint indication of a possible disk or spiral structure, but these features are very indistinct. Color gradients suggest the presence of older stellar populations dominating the galaxy's overall light profile, with a slight bluer tinge towards the outer regions, suggesting a potential for ongoing, though possibly minimal, star formation activity. No signs of major mergers or significant tidal disturbances are immediately apparent.
