The galaxy appears to be undergoing a significant interaction or merging event. It displays a disturbed morphology with a central region of concentrated light, potentially the remnant core(s) of the progenitor galaxies. Faint tidal features or extended arms are subtly visible, indicative of gravitational disruption. The overall color is bluish, suggesting the presence of younger stellar populations and ongoing star formation, particularly within the central region. The galaxy is somewhat elongated but without a well-defined spiral structure. The light distribution does not show obvious rotational symmetry. The object presents with a fairly amorphous shape, indicative of an irregular or dynamically young system that has not yet settled into a stable configuration.
