The galaxy presents as a centrally concentrated object with a smooth overall appearance. It exhibits a roughly elliptical morphology, though it leans toward a more spheroidal shape. The galaxy's light profile appears relatively uniform, lacking prominent spiral arms or a distinct disk structure. There is a subtle color gradient, shifting slightly bluer towards the center, possibly indicating a centrally located region of more recent, although subdued, star formation. The overall color index suggests the galaxy is comprised of a mix of stellar populations, with a moderate presence of older, redder stars. No major tidal features or significant morphological disturbances are readily apparent, suggesting a quiescent evolutionary history with no major recent mergers. However, close inspection reveals some slight asymmetries within the central region, suggesting possible minor disturbances. 
