The galaxy presents a largely smooth, centralized luminosity profile with a hint of lenticular morphology. It displays a dominant central bulge exhibiting a bright, yellowish-white core suggestive of an older stellar population. Fainter, diffuse extensions are visible extending outwards from the central region. The galaxy exhibits very minimal evidence of spiral arm structure. The outer regions appear to be subtly bluer, suggesting the presence of some younger stars. The galaxy has an apparently undisturbed morphology, with no signs of major tidal features or recent mergers. The shape appears closer to a circular profile than a highly elliptical one.
