The observed galaxy exhibits a clear spiral structure with two prominent spiral arms. The arms appear to be moderately wound, extending outwards from a central region. There is a hint of a bar-like structure, or a concentrated amount of stars, present in the center of the galaxy, although it is not particularly prominent. The galaxy appears relatively undisturbed, showing no strong signs of recent major mergers, though a small amount of asymmetry suggests potential minor interactions or internal disturbances. The central bulge appears relatively small in comparison to the disk, suggesting a later-type spiral galaxy. The color gradient suggests active star formation within the spiral arms, appearing bluer, and a more evolved stellar population in the central bulge region, with reddish colors.
