This galaxy presents a primarily lenticular, or possibly spiral, morphology, viewed at a high inclination angle. The primary body exhibits a smooth, centrally concentrated luminosity profile, indicating a significant bulge component. Traces of a flattened disk are apparent, exhibiting a subtle color gradient, from slightly bluer hues towards the outer regions, suggestive of ongoing, albeit subdued, star formation. There is no strong evidence of active galactic nuclei activity or a highly disturbed morphology, and there does not seem to be a clear spiral arm structure. There is no obvious indication of a recent or ongoing major merger event.
