This galaxy exhibits a disturbed morphology, indicative of an ongoing or recent merger event. The galaxy displays two distinct, partially overlapping components, each with different color characteristics. One component appears bluish, suggesting the presence of younger, hotter stars and active star formation. The other component is redder in color, indicating an older stellar population and a relative lack of ongoing star formation. The overall shape of the system is irregular and lacks a clear spiral or elliptical structure. There is evidence of tidal features and faint structures, pointing to gravitational interactions between the merging components. The spatial distribution of the light suggests a complex and dynamic system in a state of transformation.
