The galaxy presents a largely smooth, elliptical morphology. It appears nearly circular with a slight elongation. There is a faint, diffuse halo surrounding a more concentrated central region. No distinct spiral arms or bar structures are discernible. The color is generally uniform across the galaxy, suggesting an older stellar population with minimal ongoing star formation. A possible minor disturbance in the symmetry of the outer halo hints at a past interaction or minor merger event, although the overall structure remains largely undisturbed.
