The galaxy presents as a spiral type. A distinct disk structure is observed, exhibiting well-defined spiral arms. The arms appear tightly wound in some regions, transitioning to a more open structure in others. The overall color suggests an actively star-forming galaxy, particularly within the spiral arms, indicated by their blue hue. A central bulge is present, with a yellow color suggestive of an older stellar population. The galaxy appears relatively undisturbed, showing no obvious signs of a recent major merger event, though some minor asymmetry may be present. The disk is not perfectly edge-on; it presents with a notable inclination, revealing some of its spiral structure to our line of sight. A faint bar structure may be present, running through the central region, but its distinction is subtle. Two clear spiral arms dominate the shape of the galaxy, and there is no evidence of an unusually large bulge or amorphous shape. 
