The galaxy presents a clear spiral structure. The spiral arms are relatively tightly wound around a noticeable central bulge. The bulge appears to be of moderate size relative to the disk. The spiral arms show a bluer color, indicative of ongoing star formation, particularly in localized regions along the arms. Dust lanes appear to be present within the spiral arms. There is no visually apparent major merger or significant tidal disruption. The galaxy appears relatively undisturbed. There is a faint bar in the center. 