This galaxy appears to be undergoing a significant interaction, likely a merger. The primary body of the galaxy exhibits a somewhat elongated, distorted morphology, hinting at tidal forces at play. There is a clear disturbance in its overall structure.

Visually, there are at least two distinct components. A more concentrated, luminous region displays a yellowish-orange hue, possibly indicating an older stellar population or significant dust obscuration. Adjacent to this is a region of less concentrated, bluer light, potentially suggesting ongoing star formation or a different stellar population. The faint, diffuse outer regions of the galaxy show a lower surface brightness, extending further along the major axis of the system. The overall color gradient suggests spatial variations in stellar populations or dust content. The galaxy does not present a well-defined spiral structure, but does not have a completely amorphous shape either.
