The galaxy presents as a face-on spiral type, displaying a prominent central bulge that transitions smoothly into a discernible disk. While spiral arms are present, they are not tightly wound and appear somewhat flocculent and patchy in structure. The color gradient suggests a slightly bluer disk, indicative of ongoing star formation, in contrast to the yellowish-white hue of the bulge, which implies an older stellar population. There are minor distortions and disturbances in the outer regions of the disk, suggesting possible past or ongoing interactions. Overall, the galaxy exhibits a well-defined yet moderately disturbed spiral morphology.
