The galaxy presents a smooth, elliptical morphology. It exhibits a concentrated central bulge that appears yellowish-orange in color, suggesting an older stellar population. The galaxy fades outwards from the central bulge, displaying a bluer, fainter halo-like structure. This surrounding region may contain a mix of younger stars or scattered light from the central bulge. The object shows a moderately elongated shape, appearing more disc-like than perfectly spherical. No prominent spiral arms, dust lanes, or other distinct features typically associated with spiral galaxies are immediately apparent. Overall, it appears to be a relatively undisturbed, evolved system.
