The observed galaxy presents as a diffuse, irregular object. Its overall morphology suggests a system that is likely undergoing, or has recently undergone, gravitational interaction. A significant portion of the galaxy's light appears concentrated in a faint central region. Fainter light is detectable outside of this region, but does not appear to contribute significantly to the overall structure of the galaxy. There is a slight reddish color to the object, but more data are needed to confirm whether this is an indication of an older stellar population. There are signs of some minor disturbances in the overall morphology. The faintness of the galaxy suggests that it is extremely distant, and that more data is required for accurate analysis.
