The galaxy presents as a face-on spiral structure. The central bulge appears prominent and exhibits a yellow hue, suggesting an older stellar population. The spiral arms are well-defined, displaying a predominantly blue color indicating the presence of younger, hotter stars and ongoing star formation. The arms appear to be tightly wound, originating near the central bulge and extending outwards. The overall morphology suggests a possible interaction or minor disturbance. Two distinct spiral arms are visually identifiable. The galaxy does not appear to have a strong central bar structure. 
