The galaxy presents as a system exhibiting significant morphological disturbance, possibly indicative of an ongoing merger event. A primary, relatively smooth component is observed with a near-spherical morphology, displaying a predominantly yellowish-white hue with a slight central concentration. A secondary component is visible, presenting a more irregular and diffuse structure. This component shows a reddish color. The system's overall structure hints at potential tidal interactions between the two components, with possible distortions in their original shapes. This merging system has a mass comparable to our milkyway. Star formation may still be occuring, but likely at a very low rate.
