The observed galaxy presents as a complex system, potentially undergoing a merging event. There are two components, one appearing more homogenous with a slightly bluer color. The other component displays a reddish hue and seems less uniform. The shape of the system is irregular, deviating from a simple elliptical or spiral morphology. There appears to be some distortion in the overall structure, possibly indicative of tidal forces or gravitational interactions. There may be some diffuse emission surrounding the primary body of the galaxy. High resolution spectroscopic data would be helpful to determining if this system is in fact a merger.
