The galaxy presents as a somewhat elongated, diffuse structure, exhibiting a primary blue hue indicative of ongoing star formation. The central region appears more condensed, with a brighter intensity than the outer regions. The shape is roughly elliptical but not entirely smooth, hinting at potential disturbances or interactions. The overall structure suggests a moderate redshift, with the blue color possibly enhanced by its recessional velocity. There are indications of disturbed morphology which could be due to a recent or ongoing merging event.
