The galaxy presents a complex morphology suggestive of an ongoing or recent merger event. A bright, relatively compact central region is visible, potentially representing the core of one of the merging galaxies. This region exhibits a yellowish-white hue, indicating a population of older stars and potentially a significant dust component.

Extending outward from the core, a distorted disk-like structure can be discerned. This structure exhibits spiral arm-like features, albeit disrupted and asymmetric. The arms display a bluer color, implying the presence of younger, hotter stars. There also appears to be ongoing star formation in these regions.

A more diffuse, extended halo surrounds the main body of the galaxy, exhibiting irregular morphology. This halo displays a blueish tint and is punctuated by patches of brighter, concentrated light. The structure hints at tidal tails or debris resulting from the gravitational interaction between the merging galaxies. Overall, the system is significantly disturbed and lacks a clear, well-defined structure, confirming that this galaxy is undergoing significant tidal interactions.
