The galaxy presents a distinct spiral morphology. Two prominent spiral arms extend outwards from a central bulge region. These arms are loosely wound, displaying a flocculent structure with numerous star-forming regions visible as brighter knots of bluish light scattered throughout. The galaxy exhibits a relatively low inclination, allowing for a good view of its spiral structure. The central bulge appears to be of moderate size relative to the overall galactic disk. There may be a slight distortion or minor tidal feature present, though the image resolution limits definitive assessment. The disk does not appear perfectly smooth and symmetrical, suggesting some level of interaction or internal disturbance.
