The galaxy presents as a multi-component system with a disturbed morphology. There are at least three distinct, luminous clumps of material concentrated in a small region, suggesting an ongoing or recent interaction or merger. These clumps exhibit varying colors with a few areas of blueish tinges and areas of reddish hues throughout. The clumps are embedded within a diffuse, extended halo of fainter light. The overall shape appears irregular and non-symmetric, indicative of gravitational disruption. There is some evidence of tidal features, though they are not prominently defined, suggesting faint, elongated streamers extending away from the central concentration.