The galaxy presents as a small, faint object. It is likely a background object, given its high redshift.

Morphologically, the galaxy appears to lack a clearly defined disk structure. The light is generally diffuse. There is no obvious spiral structure, and no central bulge is visible. The galaxy seems to be relatively undisturbed, without strong evidence of recent major merger activity.

The color suggests that the galaxy hosts an older stellar population. The faintness of the galaxy across g, r and z bands indicates the presence of a moderate amount of dust obscuration.

Overall, this object could be an elliptical galaxy or a low surface brightness disk galaxy at considerable cosmological distance. It is possible that it is also a dwarf spheroidal galaxy. Further analysis is required for definitive classification.
