The galaxy appears to be a relatively smooth, centrally concentrated object. It exhibits a roughly circular morphology, with a slight elongation possibly present. The light profile suggests a gradual decrease in intensity from the core outwards, lacking prominent spiral arms or distinct features. The core presents a reddish-yellow hue that transitions to a more uniform pale yellow halo, indicating a predominantly older stellar population. There are no obvious signs of major mergers or significant tidal disturbances.
