The galaxy presents a complex morphology. The light profile suggests a central bulge, appearing yellowish-white, indicative of an older stellar population. Extending outward from this bulge is a faint, diffuse disk. Hints of spiral arm structure are present, though ill-defined and somewhat flocculent. Color variation within the disk suggests ongoing or recent star formation, especially towards the edges, where there appears to be bluer light. There are also faint signs of possible tidal disturbances, indicative of a past interaction with another galaxy. Overall, the galaxy appears to be undergoing some form of mild interaction or disturbance.
