The galaxy presents a generally smooth and rounded morphology. It appears to be relatively isolated, with no obvious signs of major mergers or significant tidal disturbances, though a possible minor disturbance cannot be ruled out. The galaxy's light profile suggests a centrally concentrated spheroid, characteristic of an elliptical or lenticular galaxy. The primary light component exhibits a yellowish-white hue, indicative of an older stellar population with reduced active star formation. Fainter, more diffuse outer regions are present. There appears to be a weak disk-like structure.
