The galaxy presents as a centrally concentrated object with a smooth, relatively featureless morphology. It exhibits a slight elongation, appearing more oval than perfectly circular. The core region displays a bright, yellowish hue, suggesting a significant population of older stars. There is a subtle color gradient extending outwards from the core, transitioning towards a slightly bluer tone in the outer regions. The overall light distribution is smooth and diffuse, lacking prominent spiral arms or distinct structures. There are no readily apparent signs of ongoing major mergers or significant tidal disturbances. Faint hints of what may be a disk structure are visible, though not strongly defined.
