The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The core exhibits a yellow-orange hue, suggesting a population of older stars. A diffuse, extended halo surrounds the central region, fading into the background sky. Subtle color variations are visible within the halo, indicating potential differences in stellar populations or dust distribution. No distinct spiral arms or other prominent features are readily apparent in this image, consistent with an elliptical galaxy classification. The galaxy appears relatively undisturbed, showing no strong signs of ongoing merger activity or tidal interactions with other galaxies.
