This galaxy appears to be a spiral galaxy viewed at a slight inclination. It possesses a central bulge that seems relatively small. The spiral arms are prominent, displaying a bluer hue, suggesting ongoing star formation activity. The arms exhibit a medium winding pattern, not tightly wound nor significantly loose. There is some evidence of a bar-like structure in the galactic center, although it does not appear to be very strong. The disk shows some level of disturbance, possibly due to minor interactions or internal dynamics. Overall, the galaxy does not appear to be undergoing a major merger event.
