The galaxy presents as a relatively smooth, centrally concentrated structure. It exhibits an overall elliptical morphology, appearing somewhat rounded rather than elongated. There is a distinct color gradient, with the central region displaying a more yellowish hue, potentially indicating an older stellar population. The outer regions appear slightly bluer, which may suggest ongoing, albeit subdued, star formation. No prominent spiral arms or dust lanes are discernible. The galaxy appears relatively undisturbed, without obvious signs of recent major mergers or tidal interactions. There is a suggestion of a faint, extended halo surrounding the central region.
