This galaxy presents as a relatively smooth, centrally concentrated structure. The core exhibits a yellowish-orange hue, potentially indicative of an older stellar population. A bluer halo surrounds the core, suggesting the presence of younger stars or ongoing star formation in the outer regions, although the star formation rate appears to be relatively low overall. The galaxy is not perfectly spherical, exhibiting a slight elongation or asymmetry. There is a hint of a minor disturbance or perhaps a weak tidal feature, but no clear evidence of a major ongoing merger. The morphology is primarily smooth, with subtle features. It looks like a fairly massive galaxy.
