This galaxy exhibits a well-defined spiral structure. The spiral arms are tightly wound around a central bulge. There appears to be a weak bar feature present within the central region. The bulge itself seems relatively small in comparison to the overall size of the galaxy. The disk is viewed at a slight angle, but is clearly not edge-on. The galaxy's color suggests a mix of stellar populations, with bluer regions along the spiral arms, likely indicating ongoing star formation, and a yellower central region. The spiral arm count is difficult to discern precisely but appears to be greater than two. There is no evidence of a major merger event or significant morphological disturbance but there appears to be a small disturbance to one side of the galaxy.
