The galaxy presents as a luminous, elliptical form, displaying a predominantly smooth morphology. Its central region exhibits a bright, concentrated core. A slight elongation is observed, the shape being somewhere between round and cigar-shaped. Faint, diffuse extensions emanate from the central bulge, suggestive of a stellar halo. There is no clear evidence of spiral arm structures or prominent dust lanes. The galaxy appears to be relatively undisturbed, with no major signs of mergers or tidal interactions. Color gradients suggest a possible aging stellar population, with redder hues dominating the central regions and bluer tones appearing in the fainter outer regions.
