The galaxy exhibits a spiral structure, appearing as a disk-shaped system viewed at an oblique angle. Its central region is characterized by a bright, concentrated bulge, suggesting a significant population of older stars. The spiral arms are somewhat tightly wound, displaying a bluer hue indicative of ongoing star formation. Dust lanes are visible along the inner edges of the spiral arms, contributing to the galaxy's complex structure. There is evidence of a small companion galaxy to the left that may be interacting with the larger galaxy. The overall morphology suggests a relatively massive galaxy with a moderate rate of star formation. The system does not appear to be undergoing a major merger, though there may be minor disturbances present.
