The galaxy presents a largely smooth morphology, appearing elliptical in shape. It displays a prominent central bulge, bright and concentrated, with a yellowish hue suggestive of an older stellar population. There is a subtle color gradient extending outwards from the core, transitioning to a slightly redder tone in the outer regions. No distinct spiral arms or prominent dust lanes are discernible within the observed image, indicating a lack of significant recent star formation. The galaxy appears relatively undisturbed, without obvious signs of tidal interactions or ongoing mergers. The overall light distribution suggests an evolved system with a substantial stellar mass.
