The galaxy presents a generally smooth and elliptical morphology. There is a bright, concentrated central bulge of moderate size, surrounded by a more diffuse halo. The galaxy exhibits a yellow-red hue indicative of an older stellar population and potentially dust extinction. There is no significant evidence of distinct spiral arm structures or prominent star-forming regions in the visible bands. The galaxy appears to be relatively isolated and unperturbed, with no immediately obvious signs of tidal interactions or ongoing mergers. Overall, the system appears to be a relatively massive early-type galaxy, perhaps nearing the end of its star formation activity.
