This galaxy exhibits a flattened, disk-like morphology, viewed nearly edge-on from our line of sight. There is a prominent central bulge, appearing somewhat rounded. Dust lanes are visible, obscuring the light from the disk. The galaxy shows evidence of internal structure within the disk, with hints of spiral arms. There are no obvious signs of recent major merger activity. Based on its color, the galaxy appears to have a mix of stellar populations, with some regions that are more actively forming stars.
