The galaxy presents as a relatively smooth, elliptical object with a concentrated central bulge. Its overall shape is largely circular. There is no clear evidence of spiral arms or a distinct disk structure. Color gradients suggest a population of older stars, indicated by the redder hues, particularly concentrated within the central bulge. A subtle blue component is observed, implying some recent star formation, though it does not dominate the galaxy's color profile. There is no visible evidence of ongoing major mergers or tidal disturbances, though slight asymmetry cannot be ruled out. The galaxy exhibits a well-defined central region, suggesting the presence of a supermassive black hole. Overall, this galaxy appears to be a mature, relatively undisturbed system.
