The galaxy presents a tilted disk structure. Prominent spiral arms emanate from the central bulge region, displaying a winding pattern that transitions from moderately tight to looser toward the outer edges of the disk. The arms appear continuous, with some evidence of branching or spurs. The bulge has a small to moderate size relative to the galaxy's disk and emits a yellowish light. The overall color of the galaxy indicates a mix of stellar populations. There is no obvious sign of a bar structure. The disk appears unperturbed, suggesting no recent major merger events.
