The galaxy presents as an edge-on disk galaxy. It appears as a flattened, elongated structure with a central bulge that exhibits a smoother texture compared to the disk. The bulge appears slightly boxy. There's a clear plane defining the disk, bisecting the galaxy along its major axis. Within the disk, there's subtle mottling, indicating possible dust lanes or areas of varying stellar density. The outer regions of the disk fade into the background, suggesting a gradual decrease in luminosity and stellar population density with increasing radial distance from the galactic center. No significant spiral arm structures or major merger events are apparent. Overall, the galaxy presents a relatively undisturbed morphology.
