The galaxy presents as an oblate spheroid with a discernible central bulge. There is a strong central concentration of light that fades outwards into the galactic disk. The morphology is primarily smooth, with minimal visible features suggesting spiral arms or distinct substructures. The color profile indicates a generally older stellar population, although there is a possible ringed disk of blue stars. The outer regions of the galaxy appear somewhat diffuse, which may indicate a tidal interaction or previous merger event, although no other features are noticeable.
