The galaxy presents as a face-on spiral, with a prominent disk structure. Two well-defined spiral arms emanate from a central region. These arms exhibit a loosely wound morphology. The central bulge appears relatively small, and does not dominate the overall structure of the galaxy. The arms are resolved into regions of blue, suggesting ongoing star formation activity. A slight bar-like structure is suggested. No obvious signs of major disturbance or ongoing merger activity are immediately apparent.
