The galaxy exhibits a clear spiral morphology. Two distinct spiral arms emanate from a bright central bulge region. The arms are moderately wound. There is likely a weak to moderate bar structure present, though this is difficult to discern with certainty from the image. The bulge appears to be moderate in size relative to the disk. The disk itself is the dominant feature. Based on the relatively blue hue of the spiral arms, active star formation is likely occurring. There is no visually obvious evidence of a major merger event, but some minor disturbances within the disk cannot be ruled out. The galaxy is not viewed edge-on.
