The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge that appears yellow-white in color, suggesting an older stellar population. The outer regions of the galaxy display a slightly reddish hue, possibly indicating the presence of dust or a population of cooler, redder stars. There is a faint indication of a possible disk component or some extended structure but this is hard to ascertain and the smoothness suggests an elliptical galaxy. No signs of strong tidal disturbances, major mergers, or prominent spiral arm structures are visible within the galaxy. The overall structure appears relatively undisturbed and integrated. The color gradient from center to edge might indicate ongoing, but subdued star formation at the outer regions.
