The galaxy presents as a disturbed system. It exhibits a non-smooth morphology with a complex and irregular structure. Patches of bluer light are visible within the galaxy, with hints of an extended disk. Evidence of an ongoing or recent merger is suggested by the disrupted shape, with the possibility of tidal tails or other interactive features present but not clearly resolved in this image. There appear to be regions of active star formation, inferred from the bluer coloration. The galaxy's apparent size is relatively small, potentially indicating a low-mass system or significant distance. Overall, the object appears to be a dynamically active galaxy with a history of interactions.
