The galaxy exhibits a largely smooth morphology, suggesting it is likely an elliptical or lenticular galaxy. It appears to have a concentrated central bulge, which gradually fades into a diffuse halo. There is a subtle color gradient, shifting from a yellowish-white core to a slightly bluer periphery. No distinct spiral arms or dust lanes are visible. The round, relatively featureless appearance indicates a lack of ongoing major mergers or significant star formation, although some star formation may be occurring at a very low rate.
