The galaxy exhibits a complex morphology, appearing as a system undergoing significant gravitational interaction. The overall structure is irregular and disturbed, with multiple distinct clumps or components visible. A dominant, relatively smooth and rounded component is present, exhibiting a yellowish-orange hue. This may indicate an older stellar population, likely concentrated towards the galaxy's core.

Surrounding this core are regions with a bluer color, suggesting the presence of younger, hotter stars and potentially ongoing star formation. These bluer regions are less defined and appear more diffuse. Tidal features, such as faint streams or bridges of stellar material, are suspected, extending from the main body of the galaxy. These features contribute to the overall disturbed appearance, indicating recent or ongoing merger activity. The galaxy is relatively compact in size. Overall, it seems to be experiencing strong tidal forces and merger events.
