The galaxy presents as a somewhat elongated, lenticular structure. There is a smooth, centrally concentrated bulge which appears yellow-orange in color, suggestive of an older stellar population. A faint disk extends outwards, less defined and slightly bluer in hue, potentially indicating some recent or ongoing star formation, albeit at a low rate. The disk itself does not exhibit prominent spiral arm structures. The galaxy's overall morphology suggests an intermediate stage of evolution, transitioning perhaps from a spiral towards a more quiescent elliptical form. No obvious tidal features or signs of major mergers are apparent, though subtle disturbances cannot be ruled out.
