The galaxy presents as a spiral type, with a clearly defined disk structure. Two prominent spiral arms emanate from the central region and appear loosely wound. The color of the arms suggest active star formation. The galaxy exhibits a noticeable central bulge. There appears to be a faint bar structure running through the core. The disk of the galaxy is viewed at an angle, it is not perfectly edge-on, nor face-on. There is no obvious indication of a major merger event, but some asymmetry could point to a minor interaction or disturbance.
