The galaxy presents a generally smooth and elliptical morphology. It exhibits a high Sersic index, suggesting a concentrated bulge. The axial ratio indicates it is nearly circular in appearance. Color gradients across the galaxy are present. The central region appears more luminous, transitioning to less luminous outer regions. There is no indication of prominent spiral arms or a distinct disk structure. The galaxy's color index suggests a population of older stars dominating its stellar content. Evidence indicates a relatively low rate of current star formation. No signs of major mergers are present, with no significant tidal disturbances.
