This galaxy exhibits characteristics indicative of a system undergoing a significant merger event. Its overall morphology is highly disturbed and irregular, lacking a well-defined spiral or elliptical structure. The primary body of the galaxy appears to be a diffuse, elongated structure with a yellowish hue, suggesting a population of older stars.

Notably, there are several distinct bright clumps or knots of bluish light distributed throughout the system, potentially indicating regions of active star formation triggered by the merger. Additionally, there is a smaller, more compact object with a reddish tint in close proximity, possibly another galaxy in the process of merging with the main galaxy or a tidal dwarf galaxy formed during the interaction.

The presence of diffuse tidal streams and bridges of faint light extending outward further supports the ongoing merger interpretation. These structures are formed by stars and gas being stripped away from the merging galaxies due to gravitational interactions. The overall color gradients and spatial distribution of star formation regions suggest a complex and dynamic system, consistent with a major merger event.
