This galaxy exhibits a clear spiral structure. The spiral arms are tightly wound, originating from a central, bright bulge. There is a strong bar feature visible extending across the central bulge. The bulge size appears moderate, with a relatively high degree of central concentration. The disk of the galaxy shows a subtle blue hue indicative of some ongoing star formation, although not intensely so. The galaxy is viewed close to face-on. There is no obvious indication of a major merger, though there are some minor asymmetries in the spiral arms that could suggest some gravitational disturbance.
