This galaxy appears to be a spiral galaxy with a discernible disk. There is evidence of spiral arm structure, with arms that appear to be relatively tightly wound. A bar-like structure may be present. There is a notable bulge in the central region of the galaxy, which is moderate in size. The spiral arms are well-defined, and it has a relatively high inclination. The galaxy does not exhibit any obvious signs of a major merger, although some minor disturbances may be present.
