The galaxy appears to be undergoing a significant interaction or merger event. Its central region exhibits a bright, concentrated core, surrounded by a more diffuse, elongated halo of light. This halo shows evidence of tidal distortions, with extended structures reaching out from the main body. One arm stretches significantly farther than the other. The colour profile seems to be relatively uniform throughout the main body of the galaxy, but with a bluer hue evident in the tidal features, suggesting ongoing star formation within these disturbed regions. Overall, the galaxy's morphology is highly irregular and asymmetric, indicative of a dynamically active state possibly driven by interactions with another galaxy. There is potentially a second galaxy in the top of the image.
