The galaxy presents as a barred spiral with a prominent central bulge. The bulge exhibits a yellowish-orange hue, suggesting an older stellar population. Faint spiral arms emanate from the ends of the bar. The arms appear loosely wound, extending outward from the central region. Two primary arms are visible. The overall color of the spiral arms appears bluer, indicating younger, hotter stars and active star formation regions. The galaxy shows no signs of major disruption, though subtle asymmetries in the arm structure might indicate minor gravitational interaction.
