The galaxy presents as a relatively faint, elongated structure. Its light distribution indicates it is more extended in one dimension, suggesting a disk-like or possibly spheroidal shape seen at an oblique angle. A central concentration of light is visible, likely corresponding to the galactic nucleus or bulge. Faint hints of spiral arm structure are visible on the edges. The bluer color of the disk may imply ongoing star formation, while the central region appears more yellow. There are no signs of major mergers or tidal disturbances, indicating that the system may be in a relatively isolated stage of evolution. The galaxy is compact, and the lack of bright, resolved stellar populations suggests that this object is at a considerable cosmological distance. 
