The galaxy presents as a generally smooth, elliptical-like structure with a bright, concentrated central bulge. The color gradient shifts from a yellowish-white core to a bluish outer halo. There is little evidence of spiral arm structures or significant dust lanes. The galaxy appears relatively undisturbed, with no obvious signs of tidal tails or major merger activity, though some minor distortion cannot be ruled out. The shape is somewhat elongated but not extremely so, appearing more elliptical than highly flattened. The overall color indices suggest a population of older stars in the central region, while the bluer hue in the outer regions may indicate younger stellar populations or ongoing star formation, albeit at a modest rate.
