The galaxy presents as a somewhat elliptical, concentrated structure with a smooth, diffuse halo surrounding a brighter central region. The color gradient transitions from a predominantly yellow-orange core to a blue-green outer region suggesting a difference in stellar populations. The roundness appears to be intermediate, not perfectly spherical but also not elongated. There are hints of possible minor disturbances in its overall structure, although no clear signs of major mergers or significant tidal features are apparent. The morphology is relatively smooth, lacking distinct spiral arms or prominent dust lanes. Overall, the galaxy appears to be an evolved system.
