The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits an elliptical morphology, with a high degree of radial symmetry. The light distribution suggests a dominant bulge component. Color gradients are subtle, with a slightly bluer hue in the outer regions transitioning to a redder core. There is no evidence of spiral arm structures or significant dust lanes. The galaxy appears to be isolated, without any signs of tidal interactions or nearby companions. The overall appearance indicates a galaxy that is undergoing relatively passive stellar evolution with a low rate of star formation.
