The galaxy appears to be an elliptical galaxy. It exhibits a smooth, symmetrical structure with a high degree of central concentration of light. The light profile suggests an older stellar population and a lack of significant ongoing star formation activity. There is no evidence of spiral arms or a prominent disk. The galaxy appears to be relatively isolated, with no obvious signs of recent or ongoing mergers or tidal disturbances. It has a moderate redshift, indicating that it is at a considerable cosmological distance. The shape of the galaxy is nearly circular.
