The galaxy presents a prominent disk structure. There is a noticeable central bulge region that appears moderately sized, transitioning into spiral arms. These arms appear to be wound relatively tightly around the bulge. Evidence suggests the presence of at least two spiral arms, possibly more, but this is hard to concretely determine. The arm structure seems somewhat perturbed, indicating a minor disturbance or a potential past interaction with another galactic object. The galaxy is not seen edge-on, but rather at an angle which provides a relatively full view of its structure.
