The galaxy presents as a spiral type, viewed at a significant angle of inclination relative to our line of sight. The disk is clearly visible. Two main spiral arms can be discerned, appearing somewhat diffuse and loosely wound. The galactic bulge is relatively small in proportion to the overall disk size. There is no apparent central bar structure. Overall, there does not appear to be any major merger events happening, however, there may be some minor disturbances due to its asymmetry.
