The galaxy presents as a spiral type, exhibiting a non-negligible disk component. Two distinct spiral arms are readily discernible, demonstrating a moderate winding pattern. The arms are not tightly wound, nor particularly loose, suggesting an intermediate spiral structure. A bulge is observable, occupying a moderate fraction of the galaxy's overall structure. There is no clear presence of a strong bar, although the possibility of a weak bar structure cannot be ruled out. The disk appears face-on. There are no evident signs of major disturbances, although minor disturbances are possible. The galaxy exhibits a blue hue in the outer disk and arms, while the central bulge displays a more yellow-red color. The colors indicate that the center is composed of older stars, while the outer regions consist of younger stars.