The galaxy presents as a system undergoing significant morphological disturbance, potentially indicative of a merger event. The central region appears dominated by a concentrated, yellowish population, suggesting a bulge component with older stars. A distinct bluish region is observed on one side of the core, possibly representing an area of more recent star formation or an infalling galaxy rich in young, hot stars. Extending outwards from the central bulge, faint, elongated features can be discerned, which might be tidal tails or disrupted spiral arms. The overall shape is somewhat irregular, not exhibiting a clear elliptical or spiral structure. The color gradients imply a mix of stellar populations, with the redder hues indicating older, less active regions and the bluer areas associated with ongoing or recent star formation. The inferred mass is substantial, consistent with a large galaxy.
