The galaxy presents as a barred spiral structure, viewed at an oblique angle. A prominent central bulge exhibits a yellowish-white color, suggesting an older stellar population. The spiral arms appear tightly wound and bifurcated, displaying a bluer hue indicative of ongoing star formation. Dust lanes are visible within the arms, contributing to the observed structure. The bar appears strong, bisecting the bulge. There is no apparent presence of a significant tidal disturbance suggesting any major merger event. It is a disc galaxy with a moderate-sized bulge relative to its disc.
