The galaxy presents a disk-like structure, though its orientation is not perfectly edge-on. Faint spiral arms appear to be present within the disk. The central bulge is moderately sized, with a yellowish hue, potentially indicating an older stellar population. The overall color of the galaxy is dominated by blue and green, which suggests ongoing star formation, especially noticeable in the disk. There is a reddish color on one side of the galaxy that could indicate a region of intense star formation. The galaxy also exhibits some irregularities in its structure, indicative of either tidal disturbances or a possible ongoing merger. The merging could be the cause of some of the star formation.
