The galaxy presents as a diffuse, irregular structure. There is no apparent central bulge or defined spiral arm morphology. The galaxy exhibits a clumpy distribution of star-forming regions, identifiable by their blue color, scattered throughout the galaxy's body. These regions appear to be interspersed with areas of lower stellar density. Some features suggest tidal disturbances or the presence of a faint tidal tail. Additionally, there is evidence of ongoing or recent merger activity, with disrupted morphology and visible disturbances. The galaxy appears to be relatively faint in all three color bands, indicating a moderate redshift or low intrinsic luminosity.
