The galaxy presents a spiral morphology, viewed nearly face-on. A central bulge is apparent, exhibiting a yellow hue indicative of an older stellar population. Spiral arms extend outward from the bulge, displaying a predominantly blue color, suggesting ongoing star formation. These arms appear tightly wound. There is no apparent bar structure in the central region. Faint disturbances or minor irregularities can be discerned in the outer regions of the disk, though there does not seem to be any major merging activity occuring. 
