The galaxy presents as a diffuse, extended object with low surface brightness. The morphology appears irregular, with no discernible spiral arms or central bulge. The color distribution is not uniform; it exhibits a mottled appearance with some regions appearing slightly redder than others. The overall color is indicative of an older stellar population, with less active star formation. There is a hint of possible tidal features or disturbances, suggesting a potential interaction or merger history. The edges of the galaxy fade gradually into the background sky.