The galaxy presents as a spiral structure, exhibiting prominent, well-defined arms. The morphology suggests a disk galaxy viewed at a slight angle, with a moderate-sized bulge at its center. The spiral arms appear somewhat tightly wound around the galactic center. The winding is fairly consistent, with the majority exhibiting moderate curvature. There are at least three discernable spiral arms. There is no evidence of a strong central bar structure. No significant signs of major mergers or disturbances are visible, though minor distortions or asymmetries may be present. The central bulge appears neither excessively dominant nor completely absent, showing a moderate presence.