The galaxy presents as a centrally concentrated, smooth object. It exhibits an elliptical morphology, with an axial ratio appearing close to but not quite unity. A subtle color gradient is observed, with a yellowish-white hue dominating the central region, gradually fading towards a slightly bluer periphery. This may indicate a population of older stars concentrated in the core, with ongoing star formation at the edges. There is no strong evidence of spiral arm structure or significant dust lanes. Minimal distortion suggests this galaxy is relatively undisturbed, without any evidence of major or minor mergers.
