The galaxy appears to be a relatively smooth, disk-like structure. It is seen at an oblique angle and exhibits a central bulge that is brighter than the surrounding disk. The galaxy appears slightly elongated. There is some visual evidence of a disk but no spiral structure is seen. Coloration is observed, showing the central bulge as more yellow/white, while the disk has a more blue hue, indicative of younger stars. The overall structure seems to be relatively undisturbed, with no obvious signs of a major merger. There appears to be a slight asymmetry in the outer regions of the disk.
