The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge that appears to dominate its overall structure. The color gradient suggests a primarily older stellar population, which is expected in this type of galaxy. There appears to be no significant dust lane or spiral arm structure visible in the observed wavelengths. Based on the visual appearance, it is likely a massive galaxy with a low star formation rate. No mergers or signs of major disturbances in the galaxy’s shape or stellar distribution can be observed, which also suggests that the galaxy is relaxed.
