The galaxy presents as a centrally concentrated object, appearing largely smooth in morphology. There is a slight elongation observed, though the galaxy is generally round in appearance. The color profile suggests a population of older stars, giving it a yellowish-white hue. There is no apparent disk structure or spiral arm features visible in this image. The object does not seem to be undergoing any major mergers or show signs of significant tidal disturbances. It appears as a relatively undisturbed, evolved system. The half light radius of the galaxy is approximately 5.3 kpc. The estimated stellar mass indicates this is a very massive galaxy. The star formation rate is moderate.
