The galaxy appears to be undergoing a significant merger event. A diffuse, relatively smooth component is visible, with a central concentration of light. Two distinct, brighter, and more compact structures are observed on either side of this smoother component. The color of these structures is notably redder than the central region, suggesting an older stellar population or significant dust obscuration. There is evidence of tidal features or disturbed morphology suggesting a recent or ongoing interaction. Given the presence of both smooth and disturbed components, a classification based solely on morphology is challenging. The primary body of the galaxy shows a slight elongation, deviating from a perfectly circular form.
