The galaxy presents a smooth, elliptical morphology. Its light profile appears centrally concentrated, with a gradual decrease in luminosity towards the outer regions. The core exhibits a bright, yellowish-white hue. The overall color suggests an older stellar population, possibly dominated by red giant and red dwarf stars. There is a subtle elongation in its shape, leaning toward a cigar-like form. No prominent spiral arms, dust lanes, or active star-forming regions are discernible. The galaxy appears to be relatively undisturbed, showing no signs of major mergers or tidal interactions.
