The observed galaxy appears to be a spiral galaxy, exhibiting a distinct disk-like structure. Within the disk, prominent spiral arms are clearly visible, displaying a loosely wound morphology. A central bulge is present, but it appears relatively small and not particularly luminous compared to the overall disk. A bar structure is present within the central region of the galaxy. The galaxy's color suggests a mix of stellar populations, with some regions exhibiting bluer hues indicative of ongoing star formation, particularly along the spiral arms, and other regions displaying redder colors potentially indicative of older stellar populations. The overall structure does not indicate any signs of a major merger event, though some minor disturbances cannot be ruled out. The galaxy's apparent size suggests it is a moderately sized galaxy.
