This galaxy exhibits a prominent spiral structure. Two distinct arms emanate from a moderately sized central bulge region. The spiral arms appear relatively tightly wound, displaying a medium pitch angle. The arms show evidence of active star formation, indicated by their blueish-white color. The central bulge displays a yellowish hue, suggesting a population of older, redder stars. The galaxy's disk is viewed at a slight inclination, allowing for clear observation of the spiral arm morphology. No obvious signs of a strong bar structure are apparent, nor is there evidence of ongoing major merger activity. There appears to be some minor disruption in the disk, potentially indicating minor interaction with smaller objects. The overall morphology suggests a well-defined spiral galaxy with ongoing star formation.
