The galaxy appears to be a spiral galaxy, viewed at an oblique angle, displaying a prominent disk. The disk exhibits a faint yet discernible spiral structure. The spiral arms appear loosely wound. There is evidence of active star formation within these arms, indicated by the slightly bluer hue in the spiral arms. The bulge of the galaxy appears to be of moderate size relative to the disk. There is a hint of a bar-like structure in the central region. The overall color suggests it is a relatively young and actively star-forming galaxy. There are some signs of a minor disturbance or interaction with another galaxy, but the effects are subtle and do not drastically disrupt the overall spiral structure.
