This galaxy presents as a moderately luminous, spiral-type object at a redshift suggesting a considerable distance. Its morphology appears somewhat disturbed or irregular, with a possible disk-like structure. It appears that the galaxy does not have a strong central bulge component. The galaxy exhibits a notable degree of star formation, as indicated by its blue color and faint clumpy structures. The majority of the light appears to be evenly distributed throughout the galaxy with no distinctive points of light. It is possible that the galaxy has recently experienced or is undergoing a minor merger event which would explain the irregular structures. The colors range from light blues to yellows and reds suggesting a range of star populations.
