The galaxy presents as a singular, centrally concentrated object. A bright, roughly circular nucleus dominates the morphology. The galaxy exhibits a moderate degree of overall smoothness. Some irregularities are visible, indicating a deviation from a perfectly elliptical shape. There are hints of disturbance in the outer regions of the galactic disc or halo. Based on the faint, mottled light extending beyond the central bulge, there might have been interactions with smaller galaxies, or a tidal disruption event, though this is difficult to ascertain from the current image. 