The galaxy appears as a dual-component system. The dominant, primary component exhibits a smooth, relatively round morphology. The light from this component is predominantly green and white, suggesting the presence of relatively young stars and ongoing star formation. The secondary component, positioned to the side, displays a redder hue. This coloration likely indicates an older stellar population, with a reduced rate of recent star formation activity. There may be some disturbance in the overall structure. This system may be in the early stages of a merger.
