The galaxy presents as a primarily smooth, elliptical-like structure, exhibiting a relatively round morphology. Its core region displays a concentrated, bright yellow hue, suggesting a population of older stars. There is evidence of a secondary, fainter structure exhibiting a bluish tint located closer to the galaxy's perimeter. The galaxy appears relatively isolated, with no obvious signs of recent major mergers or tidal disturbances. A hint of disk-like or irregular structure may be present within the fainter bluish region, warranting further investigation to determine the nature of any potential features. The overall color suggests that star formation rates are low.
