The galaxy presents a distinct spiral morphology. Several spiral arms are visible, exhibiting a tightly wound structure. The arms appear somewhat patchy in color distribution. A small bulge is present at the center of the galaxy, though it is not dominant. The galaxy is observed face-on, allowing a clear view of its spiral structure. There does not appear to be a strong bar feature bisecting the galaxy. The overall structure of the spiral arms suggests a relatively quiescent state, although some disturbed regions and potential indications of minor tidal interactions cannot be entirely ruled out. The color distribution indicates ongoing star formation, especially in the tightly wound spiral arms.
