The galaxy presents as a spiral type, exhibiting a disk-like structure that is not edge-on. Distinct spiral arms are visible, appearing somewhat flocculent. The arms exhibit a moderate winding, neither tightly wound nor particularly loose. The central bulge of the galaxy is present, but not dominant within the overall galactic structure, appearing to be of moderate size. A bar structure might be present within the central region, but it is not prominent. The galaxy does not appear to be undergoing a major merger, but shows some signs of minor disturbance, indicating possible past interaction with another galaxy. Star formation appears to be occurring within the spiral arms as indicated by their color and texture, but it may not be extremely vigorous at this time. The overall color suggests a population of stars with intermediate ages.
