The galaxy presents as a primarily smooth, elliptical morphology. The light distribution is highly concentrated towards the center, with a gradual decrease in luminosity radiating outwards. There is a slight elongation present, though overall it appears quite round. No distinct spiral arms or bar structures are discernible. Color gradients suggest a population of older stars, with a yellowish-white core transitioning to redder hues in the outer regions, indicative of reduced recent star formation activity. The galaxy appears isolated, with no obvious signs of tidal interactions or nearby companions. There is no dust lane apparent. There may be faint disturbances present, or it may be imaging artifacts.
