The galaxy appears as a relatively compact object with a moderate degree of internal structure. The central region presents a somewhat smooth, concentrated appearance. Fainter, extended features emanate from this core, suggesting the presence of spiral arms or tidal disturbances. There is evidence of ongoing or recent star formation activity within the galaxy, as indicated by the presence of blue-ish regions, potentially associated with younger stellar populations. Redder regions are also present, likely indicating older stellar populations and dust. Overall, the galaxy does not present a highly ordered or symmetric structure, showing a more complex, possibly dynamically active morphology. There is also a hint of an asymmetric morphology, possibly indicative of a past interaction or merger.
