The galaxy presents as a face-on spiral type. A central bulge is visible, though not particularly prominent. The presence of spiral arms is suggested, but they appear somewhat diffuse and patchy, lacking sharp definition. A bar-like structure seems to run through the central region of the galaxy. The disk component appears more dominant than the bulge. There does not seem to be any presence of tidal tails or shells which rules out any major merger events in the recent past. The overall structure seems relatively normal, with no obvious signs of major disturbances.
