The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. There is a distinct core region exhibiting a yellowish-white hue, suggesting a population of older, evolved stars. The galaxy exhibits a gradual decrease in surface brightness from the core outwards, with the outer regions appearing more diffuse and slightly bluer in color, potentially indicating the presence of some younger stellar populations, albeit at a low rate of formation. There is no evidence of strong spiral arm structure or significant dust lanes. The overall structure suggests the galaxy is relatively undisturbed, with no signs of major merging events or tidal distortions. The shape is roughly round, with a slight deviation towards an intermediate form, and is not cigar shaped.
