This galaxy appears to be an edge-on spiral galaxy, characterized by a flattened, elongated disk-like structure. A prominent central bulge is observed, with a concentration of light in the center, suggesting a relatively older stellar population. The disk exhibits a smoother texture, with a gradual decrease in surface brightness away from the central bulge. The galaxy shows no obvious signs of major disturbances or ongoing merger activity, and the disk seems relatively undisturbed. There is some evidence of internal dust lanes within the disk, indicated by subtle variations in color and brightness, which appear dark against the yellow of the galaxy.
