This galaxy presents a disturbed morphology, appearing asymmetrical and exhibiting significant tidal features. The central region demonstrates a diffuse, bright luminosity, potentially indicative of a dense stellar population or active galactic nucleus. There is evidence of potential ongoing or recent merger activity. The main body shows prominent disruptions with extended, faint plumes or tails emanating from the central region. These extensions are likely composed of stars and gas ejected during gravitational interaction with another galaxy. A substantial fraction of the galaxy's light seems to be concentrated in these disrupted regions, giving it an irregular appearance overall. Color gradients exist, with bluer hues in the central regions and slightly redder tones in the outer extensions, implying a difference in stellar populations or dust content. The galaxy appears to be undergoing significant dynamical processes that have shaped its current structure.
