The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape appears elliptical, trending towards an 'in between' classification rather than perfectly round or elongated. Color gradients suggest a redder, possibly older stellar population concentrated toward the center. Fainter, bluer hues surround the core, implying a more active star formation region in the outer areas, but at a low rate. There is no obvious evidence of spiral arm structure or a prominent disk component. The galaxy appears largely undisturbed, showing no clear indications of a major ongoing merger. There may be some slight tidal disturbances, but the overall morphology is mostly calm.
