The galaxy presents a distinct spiral structure with arms originating from a central bulge. These spiral arms appear tightly wound, and are visible to at least 2 arms. The image shows that the galaxy is not actively merging with any other galaxies or experiencing major disturbances. The bulge appears relatively small in comparison to the overall disk size. The disk appears to be presented face on rather than edge on. The color distribution suggests a presence of active star formation, particularly within the spiral arms, as indicated by the bluer hues. The redder colors present in the central bulge area may indicate a older population of stars and a lower rate of star formation. The spiral arms show a continuous structure, although there is slight variation in the arm's brightness. There is no strong central bar visible.
