The galaxy presents as a slightly tilted, disk-shaped structure. It exhibits spiral arm morphology. The arms appear somewhat loosely wound. The central bulge is prominent and exhibits a yellow-orange hue, suggesting an older stellar population. A bright area exists on the lower side of the galaxy, with another smaller area appearing in the upper right quadrant. It shows a general reddish-orange hue, with signs of possible disturbances in the morphology and likely has ongoing, but relatively low, star formation within the disk.
