The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a slight elongation. Its color is primarily yellow-orange, which could indicate an older stellar population with fewer young, blue stars. There is little evidence of significant star formation regions. The light profile suggests a centrally concentrated structure with a gradual decrease in brightness towards the outer regions. No spiral arms or a prominent disk are visible. There are no signs of active galactic nuclei or tidal tails.
