The galaxy presents as a largely featureless elliptical or lenticular object. It exhibits a high degree of radial symmetry, displaying a smooth, concentrated light profile. The galaxy appears nearly circular in projection. The central region displays a yellow-orange hue, suggesting an older stellar population with minimal ongoing star formation. No distinct spiral arms, bars, or dust lanes are discernible within the limits of image resolution. There is no clear indication of recent or ongoing major merger activity from the image. The light smoothly fades outwards from the bright nucleus.
