The galaxy presents as a relatively smooth, centrally concentrated object with a near-circular morphology. It exhibits a luminous core, surrounded by a diffuse halo of decreasing intensity. The color appears to be generally consistent across the galaxy, with a slight trend towards bluer hues in the central region. There is no readily apparent spiral structure or pronounced dust lanes. The overall structure suggests a well-evolved system, possibly an elliptical galaxy or a lenticular galaxy viewed face-on. There are no clear signs of ongoing major mergers or significant tidal disturbances, although some minor irregularities in the outer halo cannot be ruled out at this resolution.
