The galaxy presents as a moderately bright, yellowish-white elliptical system. It exhibits a relatively smooth, centrally concentrated morphology with no readily apparent spiral arms or significant dust lanes. The core appears more luminous and compact, transitioning to a more diffuse halo. There is a subtle elongation in its shape, suggesting it is not perfectly spherical. No signs of tidal tails or other major disturbances are observed, implying it is a relatively undisturbed system. The galaxy shows a general lack of distinct features, which is consistent with a passively evolving or quiescent stellar population.
