The galaxy presents as a relatively smooth, elliptical-like structure with no prominent spiral arms or bar visible in this image. It has a generally rounded appearance, although there is a slight deviation from perfect circularity. The galaxy exhibits a color gradient, with a central region appearing more yellow and a surrounding halo region that shifts toward a redder hue. No strong evidence of ongoing major mergers or tidal disturbances are observed. The galaxy is a considerable distance away, showing a significant redshift. The overall luminosity suggests a very massive galaxy. The redder color suggests older stellar populations may dominate the galaxy's composition, indicating a relatively low rate of current star formation.
