The galaxy presents as a centrally concentrated object, displaying a relatively smooth morphology with a mostly round appearance. There is evidence of some disruption in the galaxy. Color gradients are observable within the galaxy, transitioning from a reddish hue in the central regions to a yellowish-white periphery. This color variation suggests differing stellar populations and possibly dust content across the galaxy's body, with the redder areas potentially indicative of older stars or significant dust obscuration. There appear to be multiple nuclei present.
