The galaxy appears relatively compact. It presents an irregular morphology, lacking a well-defined spiral structure or elliptical shape. There is evidence of a dominant bright central region with a diffuse extension suggestive of a tidal tail or disrupted arm. The overall color seems to be consistent, though there are hints of some variation in hue within the central region, possibly indicating differing stellar populations or dust obscuration. Based on the structure, the galaxy is likely undergoing or recently underwent a minor merger, with a slight disturbance in the overall structure.
