This galaxy presents as a spiral galaxy, viewed at a significant inclination relative to our line of sight. The galaxy is composed of a central bulge which appears moderate to small in size. The spiral arms are tightly wound and possess a somewhat flocculent appearance. Dust lanes are clearly visible, obscuring some of the starlight, particularly along the near side of the galactic disk. The disk appears extended, with an overall smooth texture, indicating a relatively mature stellar population. The galaxy exhibits a bar-like structure crossing the bulge. The spiral arms extend outwards, demonstrating a significant star formation. The galaxy does not present with any signs of a major ongoing merger, but there may be minor disturbances present, affecting the morphology of the spiral arms.
