The galaxy presents as a centrally concentrated object with a smooth morphology. It is generally elliptical in shape, tending towards a circular form. The central region is bright, displaying a yellowish-white hue that suggests an older stellar population. This central brightness decreases radially outwards, transitioning to a more diffuse halo of blueish-white light. This outer halo suggests the presence of a younger, bluer stellar population, although the overall smoothness indicates limited ongoing star formation. There is no clear evidence of spiral arm structure or significant dust lanes, which would typically be found in disk galaxies. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions. Slight irregularities within the outer halo suggest possible minor disturbances.
