The galaxy presents as a centrally concentrated elliptical system, exhibiting a smooth, featureless morphology. The light profile appears regular, with a gradual decrease in intensity from the core outwards. There is no apparent disk structure or spiral arm features. The color gradient suggests a higher concentration of older stellar populations within the central bulge, transitioning to slightly bluer colors in the outer regions. The overall shape is more rounded than elongated. There is no strong evidence of any significant ongoing mergers or tidal disturbances. The galaxy appears relatively undisturbed, suggesting a dynamically relaxed state. Its estimated size places it among the larger galaxies in the observable universe. The relatively quiescent state suggests a low rate of star formation within the system.
