The galaxy presents as a spiral galaxy with a moderately inclined disk relative to our line of sight. The spiral arms are tightly wound and display a patchy, flocculent structure, indicating ongoing star formation within the disk. The central bulge is relatively small and does not dominate the overall structure of the galaxy. There may be a faint bar structure present in the center of the galaxy. There may also be a minor disturbance within the overall structure, but no obvious indication of a major merger event. The galaxy appears somewhat blueish which suggests it is still actively forming stars, but it may be old enough to have a relatively high mass.
