The galaxy presents as a fairly symmetrical, centrally concentrated system. It exhibits a smooth, elliptical morphology, lacking any discernible spiral arm structure or significant dust lanes. The core is bright and well-defined, exhibiting a bluish white hue suggesting the presence of hotter, younger stars, or possibly an active galactic nucleus. A diffuse, extended halo surrounds the core, gradually fading into the background. The galaxy appears relatively undisturbed, showing no obvious signs of major mergers or tidal interactions. There is a slight color gradient apparent, with the central region appearing bluer than the outer halo, which has a more yellow tint. This could be the result of metallicity gradients, or the presence of older stellar populations in the outer regions.
