The galaxy presents as a single, centrally concentrated object with a smooth, elliptical morphology. Its core exhibits a bright, yellowish-white color, suggesting a population of older stars and minimal dust obscuration. The intensity of the light decreases gradually with increasing radial distance from the center, with a faint halo extending outwards. There is a subtle color gradient, with the outer regions appearing slightly bluer than the core, indicating the presence of a younger stellar population than the core but still very old stars. No prominent spiral arms, bars, or other distinct features are discernible, further supporting a classification as an elliptical galaxy. The overall structure seems largely undisturbed, exhibiting no significant signs of tidal interactions or recent mergers.
