The galaxy presents a well-defined spiral structure, characterized by tightly wound arms. These arms emanate from a bright, moderately sized bulge which appears relatively smooth and concentrated. The arms exhibit a distinct blue hue, suggesting ongoing star formation activity. The galaxy's disk is viewed at a slight inclination, but not edge-on. A bar feature appears to be present, though not particularly strong. The overall structure doesn't appear to show any signs of major disturbances or mergers, but there may be a minor disturbance. Dust lanes are visible within the spiral arms, particularly on the near side. The galaxy exhibits a high degree of symmetry.
