The galaxy presents a largely elliptical morphology, appearing generally smooth and centrally concentrated. A dominant, bright core is visible, exhibiting a yellowish-orange hue, indicative of an older stellar population. Fainter, diffuse light extends outwards from the core, showing some subtle bluer patches in the outer regions. There are no clear spiral arm structures or strong dust lanes visible. Overall, the galaxy seems relatively undisturbed, although a slight asymmetry or minor perturbation in the outer halo cannot be entirely ruled out, potentially suggestive of a past interaction or minor merger event.
