The galaxy presents as a spiral type, observed at a near face-on orientation. It exhibits a prominent central bulge, with an apparent moderate size relative to the galactic disk. The spiral arms are tightly wound around the bulge. These arms are well-defined and appear to have multiple structures. The disk appears to be fairly disturbed and there is the possibility of minor galaxy merging. Dust lanes are visible within the disk, contributing to the patchy appearance of the spiral arms. The overall color profile suggests an actively star-forming galaxy, with a blueish hue indicative of younger stellar populations. There does not appear to be a strong bar structure.
