The galaxy presents a generally elliptical morphology, appearing moderately flattened with a high degree of axial symmetry. The core exhibits a high surface brightness, concentrated towards the central region. A gradual decrease in brightness is observed outward from the center, forming a somewhat diffuse halo. There is little evidence of spiral arm structure, although subtle color variations hint at potential substructures or variations in stellar population density. The galaxy's overall color index suggests a relatively evolved stellar population. The smoothness of the galaxy's light distribution indicates minimal signs of recent major merger events or significant tidal disturbances. The apparent lack of distinct features suggests a galaxy nearing a quiescent state in its evolutionary timeline.
