The galaxy presents a disturbed morphology, exhibiting characteristics suggestive of a recent or ongoing interaction or merger. Patches of dark, possibly dust-obscured, regions are observed across the galaxy’s body. It also has blue areas, implying star formation. There is a tail or stream of material extending from the main body of the galaxy. Given the apparent morphological disturbance and tidal-like feature, further investigation into the dynamics and stellar populations would be worthwhile.
