The object presents as a single galaxy, approximately 7.6 arcseconds in radius. It appears to be a spiral galaxy with no prominent central bulge, although the limited image quality makes definitive classification difficult. The arm structure is irregular and somewhat flocculent. There are no clear signs of a grand design spiral pattern. Evidence of minor disturbance or tidal features are present on the edges of the disk. There may be some evidence of a possible minor merger event occurring based on the irregular structure. Color gradients suggest active star formation regions within the arms. Dust lanes and obscuration are faintly visible within the arms. The overall color is blue-shifted, indicating the presence of younger stellar populations. There is no obvious active galactic nucleus. The galaxy is not perfectly symmetrical, possibly due to gravitational interactions.
