The galaxy presents as a concentrated, elliptical structure, with a smooth, indistinct morphology. The light profile shows a strong central bulge with a noticeable decline in luminosity moving outwards from the core. Color gradients suggest a primarily older stellar population. Little evidence of spiral arms or recent star formation is observed. Overall, the galaxy appears relatively undisturbed, showing no obvious signs of tidal interactions or major mergers. The round shape, the lack of a disk or other irregular features, and the smooth light distribution are all indications that this may be an elliptical galaxy. It exhibits a reddish hue.
