The galaxy presents a complex, disturbed morphology. It exhibits an irregular shape with notable asymmetries in its structure. Evidence of tidal features or disrupted arms indicates potential gravitational interaction with another galaxy or a recent merger event. The galaxy displays a relatively smooth central region, gradually transitioning into a more chaotic outer structure. The color distribution suggests variations in stellar populations, with bluer regions indicative of ongoing or recent star formation and redder regions potentially representing older stellar populations. The integrated color seems to be moderately blue.
