The galaxy presents as a system with significant morphological disturbance, potentially indicative of an ongoing or recent merger event. There appear to be at least two distinct components visible. One component exhibits a smoother, more diffuse profile with a yellowish hue. The second component presents a more compact, reddish morphology. The reddish hue indicates a population of older stars, possibly concentrated in a bulge or core region. The overall shape of the system is irregular, deviating significantly from a typical elliptical or spiral morphology. There seems to be a tidal feature or bridge connecting the components, further supporting the hypothesis of an ongoing merger.
