The galaxy presents as a spiral galaxy with a noticeable disk structure. The arms are tightly wound around a prominent central bulge. The bulge appears relatively bright and concentrated. The disk shows hints of dust lanes interspersed within the spiral arms. The bluer regions likely indicate areas of ongoing star formation. The galaxy appears relatively undisturbed, with no obvious signs of major merger events. A subtle bar structure is present within the central region of the disk. The overall appearance suggests a galaxy that is actively forming stars within its spiral arms, but exhibits a mature, well-defined structure.
