The galaxy presents as a spiral structure, viewed at a moderate inclination. A central bulge is apparent, exhibiting a yellowish hue. The spiral arms are relatively tightly wound, tracing a grand design pattern. Two dominant spiral arms are discernible. Evidence suggests a bar structure exists within the central region. The galaxy does not display obvious signs of a major merger, though minor disturbances might be present in the spiral arm structure.  The overall color suggests ongoing star formation is occurring within the disk.
