The galaxy presents an irregular morphology, exhibiting characteristics of a potential ongoing merger event. A luminous central region is observed, possibly indicating a high concentration of stars or active galactic nucleus activity. Extending from this central region are diffuse, disrupted structures, which may be tidal tails or debris resulting from gravitational interactions. The overall color of the galaxy appears somewhat blueish, suggesting the presence of relatively young stars and active star formation. The shape deviates significantly from a regular spiral or elliptical form, further supporting the hypothesis of a merger or significant gravitational disturbance. Faint and clumpy, there may be multiple centers, and the disk has some irregularities.
