The galaxy presents as a spiral type, viewed at a slight angle relative to face-on, but not quite edge on. It exhibits a prominent, moderately sized bulge that appears yellowish, suggesting an older stellar population. The disk is discernible and shows evidence of spiral arm structure, however, it is somewhat disturbed. The arms are fairly tightly wound. The arms display a mottled texture with interspersed blueish regions indicative of on-going star formation. The disk to bulge ratio appears somewhat high indicating that the bulge is not the prominent feature of the galaxy and the disk and arms are well developed. There are signs of minor disturbances in the galaxy's morphology, potentially suggesting a minor interaction or past merger event. Overall, the galaxy shows signs of active star formation within its spiral arms despite the developed bulge, indicating that the galaxy is still building itself.
