The galaxy presents a primarily smooth morphology, with a notable lack of distinct spiral arm structures. Its shape appears approximately elliptical, displaying a slight elongation rather than a perfectly circular form. The central region exhibits a high concentration of light, suggesting a prominent bulge component and, presumably, a supermassive black hole. The galaxy's color profile is dominated by warmer tones, indicating a stellar population that is relatively old. There are some hints of disturbances but nothing that implies this galaxy is undergoing a major merger. The overall impression is that of a relatively massive galaxy with a large population of older stars and a smooth, featureless disk.
