The galaxy presents as a relatively smooth, centrally concentrated object. It appears nearly circular in shape, with a high degree of symmetry. There's a subtle color gradient, with the central regions appearing somewhat redder compared to the outer edges, suggesting older stellar populations are centrally located, or that the color is due to dust extinction. There is no strong indication of spiral arm structure, though the galaxy is not perfectly uniform in color, which could suggest some underlying structure. There is no evidence for a major ongoing merger event, or tidal features. There may be some minor disturbance, perhaps a smaller galaxy being accreted.
