The galaxy presents as a somewhat elongated, diffuse structure. It appears to be in the midst of a significant interaction or merger event, as indicated by its disturbed morphology. There are hints of tidal tails or disrupted arms. There is not a strong central bulge. There are bright spots scattered around it, indicating potential star formation regions. The color gradient suggests a mix of stellar populations, with bluer regions possibly indicating ongoing star formation. The overall light distribution is not uniform, further supporting the interpretation of an ongoing dynamic process.
