The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. There is no discernible spiral structure. The core region exhibits a high surface brightness, fading gradually towards the outer regions of the galaxy. The overall color appears to be slightly redder, suggesting an older stellar population and suppressed star formation. The isophotes display a nearly elliptical shape. There are no indications of tidal features or significant asymmetries, suggesting it is a relaxed system and not currently undergoing a major merger.
