The galaxy presents as a relatively small, faint structure. It is visibly redshifted; showing higher presence in the r-band than the z-band. The morphology is largely smooth, with minimal indication of spiral arm features or distinct bulges. There is a slight indication of a disk component, but overall the morphology is difficult to classify, though this is likely due to the relatively high redshift of the galaxy. There is very little indication of a merging event currently occurring. The overall color of the galaxy is indicative of an older stellar population, lacking significant ongoing star formation.
