The galaxy exhibits a prominent spiral structure. Two distinct spiral arms are clearly visible, loosely wound around a central bulge. A bar structure appears present through the core. The bulge appears moderate in size relative to the overall disk. The galaxy's disk is not perfectly face-on, showing a slight inclination. Some disturbances are visible along the arm, consistent with minor tidal interactions or past merger events. The spiral arms are quite blue, indicating active star formation regions are distributed through the galaxy.
