The galaxy exhibits a pronounced spiral structure. Two primary spiral arms are discernible, tightly wound around a central bulge. This bulge is bright and appears relatively large compared to the overall galactic disk. There is a slight hint of a bar-like structure. The galactic disk shows variations in color, suggestive of differing stellar populations. Star formation regions appear distributed along the spiral arms and are visible due to their bluer tint. The dust lanes are somewhat indistinct, but their presence can be inferred from the slightly mottled appearance of the spiral arms. The galaxy's overall shape is elliptical, indicating a non-perfectly face-on orientation, but it is still relatively close to a face-on view. No major merging or tidal disturbances are immediately obvious.