The observed galaxy presents a somewhat irregular morphology. It appears as a diffuse object with a low surface brightness. The galaxy seems to lack a distinct central bulge, exhibiting a more flattened profile. Faint hints of spiral arm structure may be present, but they are poorly defined and appear disrupted. Overall color is bluish, suggestive of ongoing star formation, although redder regions are present. The galaxy shows some evidence of interaction or disturbance, possibly indicative of a recent minor merger event.
