The galaxy presents as a somewhat disturbed system, possibly undergoing a merging event or exhibiting tidal interactions. The central region displays a yellowish-white core, which is likely the bulge dominated by older stellar populations. Surrounding the core, a fainter disk-like structure is observed. The color in the disk appears slightly bluer than the core, indicating the presence of younger stars or regions of active star formation. There is a clear asymmetry in the galaxy's morphology with evidence of a significant disruption on one side, possibly indicative of an ongoing or recent interaction with another galaxy. This disruption is more pronounced and blue in color. The galaxy's shape is moderately round, though the interaction or disturbance skews it away from being perfectly spherical. Overall, this galaxy shows signs of significant activity.
