The galaxy presents as a fairly smooth, elliptical structure with a concentrated central bulge. The color gradient suggests a population of older stars dominating the core, exhibiting a yellowish-orange hue.  A faint, diffuse halo surrounds the central region, showing subtle bluer colors on the periphery, potentially indicating pockets of younger stellar populations or regions of ongoing, but limited, star formation. The overall morphology indicates a system that is relatively undisturbed and not currently undergoing a major merger. The general roundness suggests a low angular momentum system, which aligns with the observed smooth morphology.