This galaxy exhibits characteristics suggesting an ongoing or recent merger event. The overall morphology is disturbed, showing an irregular shape with luminous concentrations that could represent the remnants of distinct galactic nuclei. There's a central, brighter region, but its structure isn't clearly defined. Emanating from this central region is a diffuse, slightly elongated distribution of light. There's a hint of tidal features or extended stellar halos indicating past gravitational interactions, but the overall color is relatively homogenous. The overall hue is predominantly yellow-white suggesting an older stellar population, potentially with ongoing or recently ceased star formation. The system's overall form is indicative of a dynamic process significantly altering its structure, with signs of recent, ongoing tidal interactions. 
