This galaxy exhibits a prominent disk structure viewed at an oblique angle, oriented roughly horizontally across the image. It displays well-defined spiral arms emanating from a central bulge. These spiral arms appear somewhat flocculent, showing distinct segments rather than a smooth, continuous structure. The color gradient suggests active star formation within the arms, which are bluer in hue, and an older stellar population concentrated within the bulge, which is more yellow/red. The bulge itself is moderately sized relative to the overall disk. The disk appears to be largely unperturbed, displaying a well-defined spiral pattern without major distortions indicative of recent major mergers. There is some evidence of a bar-like structure extending from the central bulge along the major axis of the galaxy, but it is not particularly pronounced. A small amount of dust is visible within the spiral arms, showing up as slightly darker patches silhouetted against the starlight. The overall structure suggests a massive spiral galaxy with ongoing star formation and a well-defined disk morphology.
