The galaxy presents an overall disturbed morphology, potentially indicative of an ongoing or recent merger event. There is a noticeable elongation to the galactic structure. A dominant central bulge is seen, exhibiting a somewhat smooth, diffuse appearance. An arm-like structure emerges from one side of the bulge, showing areas of redder emission, which may be indicative of dust lanes or older stellar populations. Areas of bluer emission are also visible, particularly in the arm and on the opposite side of the bulge, hinting at regions of more recent star formation. Overall, the galaxy appears to be undergoing significant morphological and stellar population evolution.
