The galaxy presents as a spiral galaxy with a noticeable disk structure. The central bulge appears relatively small and moderately bright, suggesting a classical morphology. Spiral arms are clearly defined, exhibiting a tightly wound structure. The color gradient across the galaxy indicates active star formation, particularly within the spiral arms, as evidenced by the bluer hues. There are no signs of any major merging events; however, there is some evidence of minor disturbance. The disk is viewed at a slight angle, but not edge on.
