The galaxy appears as a relatively small, centrally concentrated object. It exhibits a smooth, elliptical morphology with no prominent spiral arms or disk structure immediately apparent in this image. The light distribution suggests a high degree of radial symmetry. The galaxy’s shape is roughly circular, with a slight deviation that leans towards an elliptical shape. There is no evidence of major tidal disturbances or ongoing mergers, but a faint, small region to the side of the galaxy may suggest minor disturbances or a possible faint companion. The galaxy's color appears mostly green, but this might be influenced by instrument limitations or the fact that the galaxy is very distant.
