The galaxy presents as a spiral type, observed from a near face-on orientation. Two distinct spiral arms are clearly visible, tightly wound around a prominent central bulge. The bulge is moderately sized, appearing as a bright, concentrated region. There is no indication of a strong bar structure crossing the bulge, however, there might be a weak bar. The overall appearance is that of a grand design spiral, although not perfectly symmetric. No obvious signs of ongoing major merger events or significant tidal disturbances are apparent, but minor disturbances cannot be ruled out.
