The object appears to be a galaxy at an estimated distance indicated by its redshift. It presents a somewhat diffuse morphology. There is a slight central concentration of luminosity, but the overall structure lacks a well-defined spiral arm structure or prominent disk. It is more likely a disk galaxy that is being viewed nearly face on.

The galaxy's shape is more akin to a flattened spheroid, displaying a moderate degree of ellipticity. The color index, derived from the relative brightness in different bands, indicates a population of stars that may be moderately evolved. Its estimated size is a few kiloparsecs in radius, and the total mass suggests it may be a smaller galaxy. It is possible there is ongoing minor interaction or a merging event with another galaxy.
