The galaxy appears to be an elongated, disk-shaped system viewed at a high inclination, possibly edge-on. A central bulge is visible, although not particularly prominent. Evidence of a spiral structure is present, with faint, diffuse arms extending outwards from the bulge. The arms display clumpy regions of star formation, indicated by variations in brightness and color within the disk. Overall, the galaxy exhibits a complex morphology, with possible signs of tidal disturbances or ongoing interactions, such as asymmetries within the disk and faint extensions or plumes. A merging event cannot be ruled out based on the current data. A color gradient is present, with bluer regions present near the edge of the disk.

