The galaxy presents as a relatively smooth, elliptical or lenticular structure. It exhibits a concentrated central bulge with a gradual decrease in luminosity towards its outer regions, suggesting an older stellar population. The overall color appears to be somewhat redder, potentially indicating a lower rate of star formation. There is no discernible evidence of spiral arms or a pronounced disk. The galaxy appears largely undisturbed, showing no strong signs of a recent major merger event. There is a slight asymmetry suggesting minor disturbances to the galaxy.
