The galaxy exhibits a clear disk structure with prominent spiral arms. These arms appear to be relatively well-defined and moderately wound. The central bulge is not overly prominent and blends somewhat smoothly into the disk. Overall, the galaxy displays a morphology consistent with a late-type spiral galaxy. There are no obvious signs of strong tidal interactions or major mergers, though there may be minor disturbances in the spiral arms. The color gradient suggests a higher concentration of older stars in the central bulge, while the arms show bluer hues indicative of younger stellar populations and ongoing star formation. The galaxy is not perfectly face-on, presenting a slight inclination.
