The galaxy presents a complex morphology, appearing disturbed and possibly undergoing a merging event. There are two distinct concentrations of light, one larger and more diffuse, and the other smaller and more compact. Both regions exhibit a predominantly blue color, suggestive of recent or ongoing star formation activity. The overall structure lacks a well-defined spiral or elliptical shape. There are visible disruptions and irregularities in the light distribution, potentially indicative of tidal interactions. Faint extensions or tails may be present, although they are not clearly defined. 
