The galaxy appears to be undergoing a significant interaction or merger. Its morphology is highly disturbed, displaying an irregular shape without a clearly defined central bulge or spiral arm structure. A luminous, diffuse component is visible, possibly representing tidal debris or material stripped from the main body of the galaxy during the interaction. This feature extends asymmetrically from the core, exhibiting a plume-like structure. The color gradients suggest a complex stellar population, with the presence of both older, redder stars and potentially regions of active star formation indicated by bluer components. The overall distribution of light is uneven, supporting the hypothesis of ongoing gravitational disruption.
