The galaxy presents a clear spiral structure. Two distinct spiral arms are visible. The arms appear moderately wound, neither tightly coiled nor loosely extended. There is a central bulge that is bright and moderately sized relative to the disk. A bar structure appears to be present across the center. The galaxy does not show any obvious signs of a major ongoing merger, but may have minor disturbances. The color gradient suggests active star formation regions within the disk, particularly along the spiral arms. The galaxy is viewed roughly face-on, allowing for detailed examination of its spiral morphology.
