The galaxy presents as a primarily smooth, elliptical-like structure. It appears to be quite round, with only a slight deviation from perfect circularity, lacking any readily discernible spiral arms or bar features. The light distribution suggests a concentrated central bulge with a gradual decrease in luminosity towards the outer regions, though the outer regions are hard to identify. The galaxy exhibits a generally yellowish-orange color, indicative of an older stellar population and reduced ongoing star formation. No significant dust lanes or signs of recent major mergers are apparent. There may be a smaller object in the bottom left that seems to be interacting with the galaxy, but the interaction is not strong enough to disfigure either object. 
