The subject galaxy presents a face-on spiral morphology. It exhibits a bright, concentrated central bulge, which appears yellowish-white, suggesting a population of older stars. Surrounding the bulge are loosely wound spiral arms, exhibiting a bluer hue, indicative of ongoing star formation. The spiral arms are somewhat patchy and less well-defined, giving a slightly flocculent appearance. There appear to be a few prominent HII regions visible within the arms as brighter, more intense blue knots. The disk shows a degree of asymmetry, possibly indicating a gravitational interaction or recent accretion event. A central bar is not readily apparent. The spiral arms extend a considerable distance from the central bulge, indicating a relatively large galactic disk. There are subtle indications of minor disturbances, but it's mostly a normal-looking galaxy.
