The galaxy presents a generally smooth, rounded morphology. There is a bright, concentrated central bulge that dominates the overall luminosity profile. The outer regions exhibit a fainter, diffuse halo extending outwards, with a gradual decrease in surface brightness. There may be subtle hints of underlying disk-like structure or faint arms, but they are not prominent, potentially obscured by the smoothness of the galaxy. Some minor visual disturbances are seen. Overall, the galaxy appears to be a relatively massive system, with evidence of ongoing star formation, which may be contributing to some of the disturbances, but it mostly presents characteristics of a more evolved, perhaps early-type galaxy.
