The galaxy appears to be a relatively smooth, elliptical or lenticular galaxy. It exhibits a concentrated central bulge with a gradual decrease in luminosity towards its outer regions. The galaxy displays a yellowish hue, possibly indicating an older stellar population with a reduced rate of star formation. There are no clear signs of spiral arms or significant dust lanes visible in the image. The overall morphology suggests a relatively evolved system. There are no obvious signs of major mergers or tidal disturbances in the image, suggesting relative isolation.
