The galaxy presents as a largely elliptical structure with a concentrated central bulge. The core exhibits a bright, yellowish-white hue indicative of an older stellar population. The overall shape appears to be relatively smooth and well-defined, with a high degree of symmetry. There is a subtle decrease in surface brightness moving radially outward from the core. Some faint features are visible in the outer regions, with bluer colors. There is no apparent evidence of strong tidal distortions or active galactic nuclei. The morphology suggests a relaxed system, possibly a result of past mergers or secular evolution.
