The galaxy presents a defined spiral structure. The arms appear somewhat tightly wound around a prominent central bulge. The bulge exhibits a concentrated luminosity. The disk component appears relatively smooth, with discernible spiral arms emanating from the central region. There may be some areas of active star formation present within the spiral arms. The galaxy's orientation is approximately face-on, allowing for a good view of its spiral morphology. There is a suggestion of a bar-like feature within the central region, however, it is not strongly pronounced. There is no major disturbance or indication of a significant merger event.
