The galaxy presents an elliptical morphology, appearing largely smooth and relatively undisturbed. The central region exhibits a concentration of light, suggesting a bright nucleus or bulge. The galaxy's color profile indicates a dominant population of older stars, as it appears redder compared to galaxies with active star formation. While no spiral arms or prominent dust lanes are discernible, subtle color variations may hint at minor internal structures. Overall, the galaxy's visual characteristics are consistent with a passively evolving system.
