The galaxy appears to be undergoing a merger or strong interaction with another galaxy. There are at least two distinct luminous components, possibly representing the cores of the original galaxies, with diffuse material connecting them. The overall shape is highly irregular, indicating gravitational disturbance. One of the components presents with bluer colors, potentially suggesting ongoing star formation. The other component appears redder, possibly indicating an older stellar population. Tidal tails or extended features appear to be present, further evidence of interaction. The luminosity suggests it is a relatively bright galaxy, but the diffuse appearance hints it might be a late stage merger.
