The galaxy presents as a centrally concentrated object with a smooth, relatively featureless morphology. It exhibits a dominant spheroidal component, appearing generally elliptical in shape, though slightly elongated. The core is bright and concentrated, suggesting a significant population of older stars. The color gradient transitions smoothly from a yellowish-white core to a redder halo, indicative of variations in stellar populations and metallicity with radius. There is no clear evidence of spiral arms or significant dust lanes, indicating that this system has likely exhausted most of its gas supply. A subtle, extended halo is detected, but with a low surface brightness. The galaxy doesn't appear to be undergoing any major interactions or mergers, as there are no significant tidal tails or morphological distortions visible.
