This galaxy presents a morphology that appears moderately disturbed. A central bright region, potentially the galactic nucleus, dominates the luminosity. This region appears largely featureless. Surrounding the bright center, we observe an elongated structure, suggestive of a disk galaxy seen at an oblique angle. The galaxy exhibits an asymmetrical morphology, showing some evidence of potential tidal distortions or interactions. A faint, extended halo surrounds the primary galactic structure. There is also evidence of a merging event in progress, the halo is visibly asymmetrical. There is also what may be a stream of matter emanating from the top left of the main galaxy. 
