The galaxy presents as a relatively smooth, elliptical structure, with a high degree of central concentration. The core region exhibits a yellowish hue, which potentially indicates an older stellar population, possibly dominated by evolved red giant stars. The overall form appears to be nearly circular. There are no readily apparent signs of spiral arms or significant dust lanes. A faint extended halo is visible surrounding the core, transitioning to a bluish color, which may indicate a younger stellar population. There are no clear signs of ongoing major mergers or tidal disturbances; the galaxy seems relatively undisturbed.
