The galaxy appears to be a relatively smooth, elliptical system. It exhibits a high degree of central concentration with a bright nucleus fading to a diffuse halo. The overall shape is close to circular, with minimal discernible ellipticity. There are no apparent spiral arm structures or significant dust lanes visible. Faint color gradients are noticeable, with a slightly bluer periphery compared to the central bulge which shows a redder hue. There is no clear evidence of ongoing major mergers or tidal disturbances. Faint, disturbed areas might indicate minor interactions or accretion events.