The galaxy presents a distinct spiral morphology. Two well-defined spiral arms emanate from a moderately sized central bulge. The spiral arms appear relatively tightly wound near the core and begin to loosen as they extend outward. The color distribution within the galaxy indicates a concentration of older stars within the bulge, displaying a yellowish hue. Conversely, bluer regions observed along the spiral arms suggest ongoing star formation. The galaxy exhibits a relatively ordered structure, with minimal signs of major gravitational disturbance. The disk is close to face on, with only a very slight inclination. There is no strong bar structure visible in the galaxy's center. The spiral arms have high definition, indicating a high degree of star formation is present.
