This galaxy appears to be a spiral galaxy oriented approximately edge-on to our line of sight. The central bulge is prominent and exhibits a yellowish-white hue, suggesting an older stellar population. Faint spiral arms extend from the central bulge, showing a bluish tint indicative of ongoing star formation. The arms are loosely wound, and two dominant arms can be observed, tracing along the longer axis of the galaxy. There is some asymmetry or minor disturbance visible within the spiral arms, which suggests a possibility of minor gravitational interaction with another galaxy or that the galaxy is undergoing internal structural changes. Dust lanes are present along the plane of the galaxy, obscuring some of the light from the bulge and the spiral arms.
