The galaxy presents as a spiral, observed at an oblique angle relative to our line of sight. It displays a prominent, elongated central bulge, indicating a concentration of older stellar populations. The disk component is clearly visible, though it exhibits a relatively smooth texture. There are spiral arms exhibiting a tightly wound morphology, and a relatively large, central bulge. The inclination of the galaxy reveals that the plane of the disk is significantly tilted with respect to our viewpoint, which obscures some of the detailed structure within the spiral arms. 
