The galaxy appears as a centrally concentrated object with a largely smooth morphology. The light profile suggests a spheroid-dominated system. There is a subtle color gradient visible, with the core exhibiting a yellowish-white hue, possibly indicating an older stellar population. The outer regions appear slightly redder. No distinct spiral arms or bar structures are discernible. Based on its appearance, the galaxy is likely an elliptical, or possibly a lenticular, galaxy at intermediate redshift. There are no obvious signs of recent major merger activity or strong tidal interactions. The overall structure is relatively undisturbed.
