The galaxy presents as an elliptical or lenticular type. It appears largely smooth and centrally concentrated, with a bright, yellowish core region indicating an older stellar population. A fainter, diffuse halo surrounds the core. There is some suggestion of a disk-like structure, but the image does not resolve any clear spiral arms. Some subtle color variations are present in the halo, perhaps indicative of regions of ongoing or recent star formation. No obvious signs of tidal disturbances or ongoing mergers are apparent. The overall morphology suggests a galaxy that is relatively evolved and dynamically relaxed.
