The galaxy exhibits a spiral morphology. The galaxy's light is dominated by the features in its disk. The structure of the disk features loosely wound spiral arms that appear to emanate from a relatively small, moderately bright central bulge. There are two dominant arms. Some regions of these spiral arms show a bluer tint, suggesting ongoing star formation. The galaxy appears overall symmetric with only minor disturbances in its structure. A faint bar structure is present traversing the central bulge, and has a generally similar alignment to the direction of the arms. The overall color of the galaxy suggests an intermediate age stellar population.
