The galaxy exhibits a prominent, moderately bright central bulge that gradually fades outwards into a disk structure. The disk is not perfectly face-on but inclined, with the major axis extending horizontally across the image. The spiral arms are visible, tightly wound around the central bulge, indicating a possibly older or more gravitationally stable structure. The colour of the galaxy suggests it is actively forming stars, the blue colour indicates active star formation and relatively little dust. There also appears to be little indication of any major interaction or merger events currently affecting this galaxy.
