This galaxy presents a spiral morphology with a disk that is not viewed completely edge-on. There appears to be distinct spiral arm structure. The disk exhibits a blue hue, suggestive of ongoing star formation. A bar structure is present. A central bulge is discernible, but not dominant. No major signs of an ongoing merger are visible, though some minor disturbances cannot be ruled out. Overall, the galaxy appears to be a relatively undisturbed spiral galaxy undergoing active star formation within its disk.
