The galaxy presents a generally smooth and elliptical morphology, with a concentrated central bulge. The light distribution appears relatively uniform across the galaxy, suggesting a lack of prominent spiral arms or distinct features. The galaxy's color gradient indicates a redder core transitioning to slightly bluer outer regions, potentially implying a mix of older stellar populations in the center and younger stars in the outskirts. There is a subtle asymmetry visible, possibly indicating a minor gravitational interaction. The overall form suggests a galaxy that is relatively evolved, with ongoing, but subdued, star formation.
