This galaxy presents as an irregular system, showing evidence of significant gravitational disturbance. The morphology suggests an ongoing or recent merger event. One section of the galaxy appears relatively smooth and compact with a bright, almost stellar-like core. Connected is a less concentrated area, with hints of disrupted structures that could potentially be tidal tails or distorted spiral arm remnants. This less concentrated part displays bluer color, possibly indicating recent star formation. Redder regions are present. Overall, the galaxy's appearance points towards an interaction-driven evolution, likely a major merger, reshaping its original structure. The system is not particularly large and appears to be at an intermediate distance.
