The galaxy presents a flattened, disk-like morphology, observed nearly edge-on. It exhibits a smooth, relatively featureless structure, with no distinct spiral arms or bar visible. The overall color appears to be slightly redder, with a hint of bluer color towards the edge, suggesting older stellar populations dominate, although some star formation may occur in the disk. No signs of active galactic nuclei or strong starburst activity are apparent in this image. There is some morphological disturbance, which may be from the beginning stages of a galaxy merger. It has an intermediate roundness and a moderate mass.
