The galaxy appears as a centrally concentrated, spheroidal object with a smooth light profile. The core exhibits a bright, yellowish-white hue, suggesting a population of older stars. Moving outward from the center, the color transitions to a slightly bluer, less intense halo. There is no discernible spiral arm structure or dust lanes visible in this image. The overall roundness and lack of significant disturbances indicate a relaxed morphology, with no immediate signs of ongoing major mergers or tidal interactions. The relatively compact nature of the object implies a high degree of central mass concentration. The color gradient suggests some ongoing star formation, though possibly at a low rate.
