The galaxy presents as a system undergoing a possible merger or significant tidal interaction. It exhibits an irregular morphology, lacking a well-defined spiral or elliptical structure. There are two distinct, concentrated regions of light. One appears somewhat bluer in color, suggesting the presence of younger, hotter stars within. The second region shows a comparatively redder hue, indicating potentially older stellar populations or significant dust obscuration. A faint bridge of material appears to connect these two regions, but the connecting bridge is very ambiguous. The overall form is disturbed, showing hints of tidal tails or extended stellar streams, although these are faint.
