This galaxy presents as a relatively compact and concentrated object. Its overall form is elliptical, with a smooth, diffused light profile, suggesting a significant population of older stars. The central region exhibits a slight reddish hue, potentially indicating a higher concentration of older, cooler stars or dust obscuration. Fainter bluish extensions are observed around the core region, possibly indicating a relatively low level of recent star formation. No prominent spiral arms or distinct features are apparent. The galaxy does not show any obvious signs of major disturbances or mergers. It appears to be a relatively undisturbed, evolved system.
