The galaxy presents as a smooth, elliptical form with a dominant central bulge. The light distribution is concentrated towards the core, which exhibits a yellowish-orange hue, suggesting an older stellar population. The outskirts of the galaxy are less defined and gradually fade into the background sky. The overall color gradient implies a lack of significant recent star formation throughout the galaxy. There are no visible spiral arms or dust lanes. The galaxy appears relatively undisturbed, showing no clear signs of ongoing mergers or tidal interactions. Its elongation suggests it could be classified as an elliptical galaxy of type E4 or E5 on the Hubble sequence.
