The galaxy exhibits a complex morphology, with a dominant, relatively smooth central component. The overall shape appears slightly elongated rather than perfectly circular. A clear disturbance or interaction is present, with indications of a possible merging event. A brighter, more compact region shows a distinct color difference in comparison with the larger and diffuse component. The colour variation may imply differing stellar populations and activity levels within the galaxy. There is possibly a faint feature in the form of a plume or tidal tail extending from the central region.
