The galaxy presents as a centrally concentrated, elliptical morphology with a smooth light distribution. The object exhibits a prolate shape. There is a color gradient, with the core appearing more yellow, possibly indicating an older stellar population and less ongoing star formation towards the center. The outer regions appear redder. There is no clear evidence of spiral arm structure or a distinct disk component. The galaxy appears undisturbed, showing no signs of recent major merger activity. The object has a moderate estimated size, as can be determined from the image.
