The galaxy presents as a relatively smooth, elliptical morphology. A bright, concentrated central bulge dominates the galaxy's structure. The light distribution appears centrally condensed, with a gradual decrease in surface brightness moving outward from the core. The core exhibits a yellow-orange hue, potentially indicative of an older stellar population, while the outer regions show a bluer tinge, suggesting the presence of some younger stars and potentially ongoing, low-level star formation. There's no clear evidence of spiral arms or a prominent disk structure. The galaxy appears largely undisturbed, showing no major signs of ongoing or recent mergers, though there may be some slight asymmetries. The overall shape appears mostly circular.
