The galaxy appears to be a luminous elliptical, exhibiting a smooth, relatively featureless morphology. Its shape is somewhat in between round and elliptical, with a slight elongation. The galaxy displays a prominent, concentrated central bulge that dominates the light output, and a more diffuse halo surrounding it. There is a visible color gradient with the core appearing yellower than the outer regions. The light distribution suggests that the galaxy is relatively undisturbed, showing no signs of major merger activity or significant tidal distortions. The absence of readily identifiable dust lanes or spiral arm structures indicates that the galaxy has a low rate of star formation and is likely composed predominantly of older stellar populations.
