The galaxy presents as an elliptical morphology, displaying a smooth, relatively featureless appearance without discernible spiral arms or significant dust lanes. It exhibits a concentrated central bulge that gradually fades into a diffuse outer halo. The light distribution is somewhat elongated, deviating slightly from perfect circularity and suggesting a possible oblate spheroid shape. There is no clear indication of an active galactic nucleus or intense star-forming regions. The overall color is moderately red, suggesting a stellar population dominated by older, cooler stars and a low rate of current star formation. No evidence of any major merger events is present.
