The galaxy presents a distinct spiral morphology. Two prominent spiral arms emanate from a central bulge region, displaying a loose winding pattern. The arms appear relatively smooth and well-defined, with subtle variations in color suggestive of differing stellar populations or dust distribution. The central bulge appears moderately sized compared to the overall disk. There is no sign of a strong bar structure. The galaxy displays a slight inclination relative to our line of sight. Overall, the galaxy shows no indications of major disturbances or ongoing merger activity.
