The galaxy exhibits a distinct spiral morphology. The spiral arms appear well-defined, displaying a flocculent structure. The winding of the spiral arms is intermediate, neither tightly wound nor exceptionally loose. There are approximately 3 spiral arms. The bulge component is moderately sized relative to the disk and possesses a yellow hue. The disk component appears to be undergoing active star formation, evidenced by its blue color and patchy distribution of luminous regions. No major disturbances indicative of a recent major merger event are apparent. The galaxy is viewed at a slight angle, and it is not edge on. 
