The galaxy presents a disk-like structure, with evidence of spiral arm features. The central bulge appears prominent and has a smooth texture, exhibiting a yellow-orange hue, suggesting an older stellar population. The spiral arms are not tightly wound, appearing more open and somewhat flocculent. These arms display a bluer color, potentially indicating on-going star formation. There is a slight asymmetry in the overall morphology, with one side appearing more extended or disturbed compared to the other. A minor degree of interaction or disturbance cannot be ruled out based on this image alone. The color gradient suggests a radial change in stellar populations, with older stars concentrated in the bulge and younger stars distributed in the arms.
