The galaxy presents as a single, centrally concentrated object. It exhibits a smooth, elliptical morphology with a noticeable color gradient. The core region appears bright and yellowish-white, indicative of an older stellar population. Moving outward from the center, the color shifts subtly towards a reddish hue, potentially signifying a decreasing age gradient in the stellar populations or increased dust extinction at larger radii. Faint hints of extended structure, though subtle, suggest the presence of a diffuse halo surrounding the main body. No distinct spiral arms or bar structures are discernible. The galaxy's overall form suggests a mature system with minimal ongoing star formation. Subtle asymmetries hint at the possibility of a minor gravitational interaction or past merger event, though the dominant visual impression is one of a relatively relaxed and well-mixed system.
