The galaxy presents as a merging system or a galaxy experiencing significant tidal disturbance. The primary body exhibits a concentrated central region with an apparent color gradient shifting from yellower hues in the core to bluer tones in the outer regions. A secondary, less defined structure extends from this central area, suggesting a possible interaction or merger. The overall morphology deviates from a smooth elliptical shape, indicating substantial disruption of its gravitational equilibrium. There's evidence of ongoing or recent star formation activity, particularly noted in the bluer regions, possibly triggered by the gravitational interaction.
