The galaxy presents as a spiral type, exhibiting distinct spiral arms. It displays a moderate central bulge. The arms appear to be relatively tightly wound. There is a suggestion of a bar-like structure traversing the bulge. The galaxy exhibits a blueish hue. This suggests it is actively forming stars. It appears not to be undergoing any major interaction or merger, as its structure is relatively undisturbed, although some minor disturbance cannot be fully ruled out.
