The galaxy presents as a centrally concentrated object with a smooth, featureless appearance. The light profile suggests a spheroidal morphology, likely an elliptical galaxy or a lenticular galaxy viewed face-on. The core exhibits a bright, concentrated luminosity, gradually diminishing outwards. The color index, inferred from the bluer inner regions transitioning to redder outer regions, suggests a possible aging stellar population with ongoing star formation centrally located. No apparent spiral arms, dust lanes, or other distinct features are visible within the galaxy's structure. The overall shape approximates a slightly elongated ellipse, with no obvious signs of tidal disturbances or ongoing mergers, although minor disturbances cannot be ruled out at this resolution.
