This galaxy exhibits a clear spiral structure. Two prominent arms emanate from a bright, concentrated central bulge. The arms appear relatively tightly wound, and the overall color of the galaxy suggests active star formation, particularly in the spiral arms, which show a bluer hue. The bulge appears yellower, indicating an older stellar population. The disk is viewed at an oblique angle, providing a partial but clear view of the spiral morphology. There may be a weak bar structure in the center. There is little evidence of any major mergers or significant disturbances in its shape. The galaxy displays a classic spiral form with a dominant disk and moderate-sized bulge.
