The galaxy presents as a relatively faint and small, likely distant, object. Its morphology appears disturbed. There is a very low probability that it could be a smooth galaxy, as indicated by its elongated and irregular structure. There appears to be minor disturbance in the disk, suggestive of a possible interaction or past merger event, though the possibility of it being an active merger is low. The galaxy displays a diffuse, amorphous shape, and some asymmetry. No clear spiral arms or a well-defined galactic bulge are observable. Its color indices suggest a range of stellar populations within the galaxy. The overall appearance indicates a galaxy that is in a state of disruption, or could be undergoing formation. Further spectral analysis is necessary to determine its redshift, star formation rate, and age. 
