The galaxy presents a distinct spiral morphology. The disk is oriented at a moderate inclination, offering a partial view of its structure. Two prominent spiral arms emanate from the central region, exhibiting a relatively open, loosely wound configuration. A bar structure is present within the galactic nucleus, appearing somewhat strong. The bulge size is notable, occupying a significant portion of the galactic center, but doesn't quite dominate. There's no evidence of a major ongoing merger; the galaxy appears relatively undisturbed, potentially exhibiting minor asymmetries. Overall, the galaxy is a spiral type displaying characteristics of ongoing star formation in its arms, inferred from the color variations within the structure.
