The galaxy presents as a disturbed system, exhibiting a non-uniform, asymmetrical morphology. There is evidence of an interaction or merger event. The galaxy appears to be in the intermediate stages of such an event. The central region of the galaxy has a relatively smooth appearance, with a bright core. Emanating from this central region are extended, diffuse features, possibly tidal tails, indicative of gravitational disruption. These features display a bluer hue compared to the central region, potentially indicating ongoing or recent star formation activity within these disrupted structures. The overall shape deviates significantly from a typical elliptical or spiral structure, supporting its classification as an interacting or merging galaxy.
