The galaxy appears to be a relatively smooth, elliptical system. The core exhibits a concentrated, bright region, suggesting a significant stellar density. The overall color profile indicates a population of older stars, with a notable absence of strong blue emission typically associated with active star formation. Subtle color gradients may indicate some structural features within the galaxy, though higher resolution imaging would be required to confirm this. There is a slight chance of a minor disturbance in its form, but mostly shows a smooth structure. The light profile appears well-rounded, with a minor extension to the side. Based on its estimated distance, it is likely a large galaxy with a considerable stellar mass. It displays a low specific star formation rate.
