The galaxy presents a primarily smooth morphology, exhibiting a concentrated central bulge. Its shape is largely round, with a minor deviation toward an elliptical form. There is little evidence of spiral arm structure. The galaxy displays a color gradient, shifting from a yellowish core to a bluer outer region. The color suggests older stellar populations dominating the core, with possible ongoing, albeit limited, star formation at the periphery. The galaxy does not appear to be significantly disturbed or undergoing a major merging event.
