The galaxy presents a spiral morphology, viewed at an oblique angle, but not quite edge-on. Spiral arms are readily apparent, exhibiting a multi-armed structure. The arms appear relatively tightly wound in some regions, with varying degrees of dispersion throughout the galaxy. Star formation appears to be active, indicated by the generally blue hue. A moderate bulge is visible. There are indications of potential gravitational interactions, exhibiting minor disturbances. The disk is not perfectly smooth, showing clumpy regions. There is no strong central bar, and the disk appears to be the dominant morphological feature. The galaxy is not undergoing a major merger.
