The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape is elliptical, exhibiting a high degree of roundness. There is a distinct color gradient, with a reddish-yellow hue in the core transitioning to a greenish-blue tinge in the outer regions. This color variation could indicate differences in stellar populations or dust content across the galaxy. There are no obvious signs of spiral arm structures or significant tidal disturbances. Based on its morphology, the galaxy appears to be a relatively undisturbed system with ongoing, but moderate star formation.
