The galaxy presents as a spiral type, exhibiting a disk structure that is not viewed edge-on. There is evidence of spiral arms. A central bulge appears present but does not dominate the galaxy's overall luminosity. A bar structure may be present; if so, it appears faint. Star formation activity seems to be present within the disk, though not at an extremely high rate. There is no clear visual evidence of a major ongoing merger, but minor disturbances might be present, although this is uncertain.
