The galaxy presents as a somewhat diffuse object, exhibiting a centrally concentrated light profile. Its overall color suggests a moderate amount of star formation, with a bluer hue compared to ellipticals, although it's not intensely blue like actively star-forming spirals. The galaxy displays spiral arm structures, as suggested by the disk-like appearance, that are not tightly wound and appear somewhat disrupted. It also shows signs of possible tidal features or distortions. In its overall morphology, there are signs of a potential ongoing or recent interaction or merger event. The shape is not perfectly elliptical, indicating a significant disk component. There are also areas of both smoother light distribution and areas that show clumpy features possibly representing stellar nurseries or dust lanes.
