The galaxy presents a disk-like morphology, viewed at a slight angle relative to edge-on. Spiral arm structure is clearly visible, with a high degree of arm coherence and grand design. The arms appear relatively tightly wound and extend noticeably outwards from the central bulge. The central bulge appears small, with an elliptical shape, indicating a small contribution to the overall light. The disk component is dominant, with a distinct and prominent feature in the form of organized, dusty spiral arms. The galaxy exhibits a relatively high degree of symmetry. There are no indications of tidal distortions or recent merger events. Star formation is likely ongoing within the spiral arms, giving rise to the observed bluer color gradient.
