The galaxy presents as a luminous, elliptical-like structure. Its morphology is predominantly smooth, with a highly concentrated central bulge that transitions into a fainter, diffuse halo. The color gradient suggests an aging stellar population, with a yellowish-orange hue dominating the central regions, indicative of older, redder stars. There is a subtle suggestion of bluer color at the fringes, potentially indicating some ongoing, albeit minimal, star formation activity in the outskirts, which may be caused by tidal activity that is not easily visible. No distinct spiral arms or prominent dust lanes are observed. The overall appearance indicates a galaxy that is relatively undisturbed.
