The galaxy presents as a smooth, centrally concentrated object with a predominantly elliptical morphology. The core exhibits a bright, yellowish-white hue, suggestive of an older stellar population. A more diffuse, greenish-yellow halo surrounds the central region, possibly indicating the presence of a younger stellar population or ongoing star formation, albeit at a low rate. There is no clear evidence of spiral arms or a disk structure, and it appears to be undisturbed, with no major signs of tidal interactions or merging activity. The overall structure indicates a relatively evolved galaxy, likely an elliptical or lenticular type, at a considerable distance.
