The galaxy presents as a relatively smooth, centrally concentrated object. The light distribution indicates a spheroidal morphology, likely an elliptical galaxy. There is a slight elongation, though the overall shape is nearly circular. The central region exhibits higher brightness, suggesting a dense core. The galaxy appears relatively isolated, showing no obvious signs of major interactions or ongoing mergers. There's a subtle color gradient, shifting from a bluer hue in the central region to redder tones in the outer regions, possibly indicating differing stellar populations or dust content across the galaxy. Star formation appears to be taking place at a moderate rate.
