The object appears to be a galaxy, generally elliptical in shape. The central region presents a high degree of luminosity, concentrated in a relatively small area. The light from the central bulge appears yellowish to orange in color, potentially indicating an older stellar population. Proceeding outward from the center, the light diffuses, and the color is not as intense. The overall structure is mostly smooth, and the galaxy does not appear to be heavily disturbed. The galaxy is relatively round, with minimal elongation observed. No strong evidence of spiral arms or a distinct disk structure is observed. It shows a degree of symmetry and does not appear to be undergoing a major merger event, although there are hints of a minor disturbance on one side.
