The galaxy presents a generally smooth, elliptical morphology. It exhibits a slightly elongated shape, tending toward a more oblate rather than perfectly spherical form. There appears to be a distinct color gradient, with the central region displaying a reddish-orange hue, possibly indicating an older stellar population. The outer regions have a more blueish-green appearance, which could suggest the presence of younger stars or ongoing star formation, although the image resolution makes it difficult to confirm distinct spiral arms or features. There appears to be only a small amount of visible dust.
