The galaxy presents as a relatively smooth, elliptical structure. It exhibits a concentrated central bulge that dominates its overall appearance, with a gradual decrease in luminosity outward from the center. The galaxy displays an orange-red hue, which is indicative of an older stellar population, with little evidence of recent star formation. There appears to be a lack of distinct spiral arms or prominent dust lanes; thus, it's most likely an elliptical galaxy. There is a slight elongation, moving from the bottom left to the top right of the galaxy, rather than being perfectly circular. Overall, the galaxy appears to be relatively undisturbed, lacking obvious signs of a major merger event.
