This galaxy presents as a spiral type, exhibiting prominent spiral arms that appear tightly wound. The galaxy's disk is inclined relative to our line of sight, presenting a flattened, oval appearance. A central bulge is visible, appearing relatively moderate in size and luminosity.

There is some indication of a bar-like structure in the center, although it is not strongly defined.

The spiral arms show some asymmetry, with the suggestion of tidal distortion. The spiral arms have a two-arm structure, and appear to be relatively continuous. There is no obvious evidence of a major merger, but potentially a minor disturbance.
