The galaxy presents as a somewhat amorphous, though generally elliptical, structure. The central region exhibits a high surface brightness with a yellowish-white hue, suggesting a population of older stars. Extending outward from this bright core is a more diffuse halo. Within the halo, there appears to be a region of active star formation characterized by a reddish tint on one side of the galaxy. This reddish hue is indicative of ionized hydrogen gas and the presence of young, hot stars. The overall structure suggests a galaxy that is either a relatively undisturbed elliptical galaxy with recent or ongoing minor star formation, or a galaxy undergoing a minor merger event.
