The observed galaxy appears to be an interacting system, possibly in the early stages of a merger. A central bright region is visible, surrounded by a more diffuse halo. Extending from this central region are what appear to be tidal features or distorted arms. There is an indication of asymmetric structure, with one side showing a more elongated and disturbed morphology than the other. The color distribution suggests a gradient, potentially indicating variations in stellar populations or dust content across the galaxy. There may be possible evidence of a merging counterpart, as indicated by the irregular shape. Artifacts are noted. Overall, the galaxy exhibits features consistent with an ongoing interaction and tidal disturbances.
