This galaxy exhibits a prominent disk structure and is viewed at an oblique angle, meaning it is neither face-on nor edge-on. The morphology is indicative of a spiral galaxy with well-defined spiral arms. The arms appear tightly wound, tracing a distinct pattern as they emanate from the central region. 

The central bulge appears relatively small to moderate in size and presents a yellowish-white hue, possibly indicative of an older stellar population. The disk component displays a bluer color, particularly in the spiral arms, suggesting ongoing star formation. There is no obvious central bar feature. No signs of major disturbances or interactions with other galaxies are apparent in this image, but there could be minor disturbances. The galaxy appears reasonably symmetric and well-formed.
