The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. It exhibits a predominantly yellow-orange color, indicating an older stellar population with fewer young, blue stars. The light distribution is relatively uniform, lacking prominent spiral arms or distinct features. The shape is close to round, showing minimal elongation. There is no obvious sign of active galactic nuclei activity, tidal features, or major disturbances suggestive of recent mergers, although minor disturbances cannot be ruled out. Overall, the galaxy likely has a high mass and low star formation rate. 
