The galaxy presents as a spiral with a moderate bulge. The spiral arms are prominent, well-defined, and display a primarily two-arm structure. These arms exhibit a medium winding pattern. There is a strong indication of a bar feature traversing the galactic center. The color profile suggests active star formation within the disk, with bluer hues concentrated along the spiral arms and a yellower color in the central bulge. The disk appears relatively undisturbed, showing no major signs of a significant merger event, although there are minor disturbances. The galaxy is not viewed edge-on.