The galaxy exhibits a complex morphology, appearing to be undergoing some form of interaction or disturbance. The primary body of the galaxy presents a diffuse, somewhat irregular structure. There is a slight indication of a disk-like component, but it is not well-defined. The color distribution is not uniform across the galaxy. There is a hint of a faint tidal tail or extended structure emanating from the main body, suggesting a possible merger or interaction with another galaxy. There are some regions within the galaxy that exhibit slightly enhanced star formation activity, indicated by the subtle variations in color. Overall, the galaxy's morphology suggests it is not a quiescent, isolated system. It seems to be actively evolving under the influence of external gravitational forces.
