The galaxy presents a disk-like structure with prominent spiral arms. The arms are relatively tightly wound. It possesses a central bulge, estimated to be of moderate size relative to the disk. The galaxy is viewed at a slight angle, not completely face-on or edge-on. There is no evidence of any major ongoing merger event or significant tidal disturbance, but possible minor distortions or interactions cannot be excluded. A stellar bar may be present in the central region, but it does not appear to be strongly defined. The overall color is a mixture of blue and red, suggesting a combination of ongoing star formation in the arms and an older stellar population in the bulge. 
