The galaxy presents as a centrally concentrated, largely featureless object, likely an elliptical or lenticular galaxy given its smooth appearance. It exhibits a roughly circular morphology with no distinct spiral arms or bar structure visible. The color profile suggests an older stellar population, with a reddish core transitioning to bluer hues in the outer regions, indicative of potential residual or ongoing, albeit low-level, star formation. The overall shape appears undisturbed, showing no major signs of recent or ongoing mergers, though subtle asymmetries or minor disturbances cannot be ruled out. The galaxy appears relatively compact.
