The galaxy presents as a smooth, elliptical morphology. The light distribution indicates a high degree of central concentration, with a gradual decrease in surface brightness moving outwards from the nucleus. There is a slight elongation in its overall shape, hinting at a classification that is not perfectly spherical but rather somewhat cigar-shaped. A slight blue tinge is noted in its outer regions, which may suggest ongoing, albeit mild, star formation activity. The galaxy appears relatively undisturbed, showing no obvious signs of major mergers or significant tidal interactions.
