The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge that dominates the overall luminosity profile. The light profile appears to gradually fade from the center outward, with no distinct spiral arm structures or prominent dust lanes visible. There is a slight color gradient observed, with the central region displaying a warmer, yellower hue, possibly indicative of an older stellar population. The outer regions tend towards a cooler, bluer color, potentially suggesting some ongoing, albeit limited, star formation. The overall symmetry is remarkably undisturbed with no obvious signs of recent or ongoing mergers. The galaxy's structure appears to be well-relaxed and unperturbed.
