The galaxy exhibits a disk-like morphology, viewed at a moderately inclined angle. Spiral arm structures are present but somewhat flocculent and tightly wound, extending outwards from the central region. A central bulge is apparent, though not dominating the overall structure. The galaxy appears to be slightly barred. The color distribution suggests ongoing star formation within the spiral arms. Overall, the galaxy appears to be a spiral galaxy with moderate star formation and no major signs of interaction.