The galaxy presents an irregular morphology, with a flattened, elongated structure. There is no defined nucleus or spiral arm structure readily apparent. Instead, the galaxy appears clumpy, with several distinct regions of enhanced luminosity. These brighter regions are yellowish-white in color, suggesting populations of older stars. The overall color of the galaxy appears redder than typical spiral galaxies. The lack of significant blue emission indicates a low rate of ongoing star formation. The galaxy appears to be undergoing some form of disturbance, which is possibly caused by an interaction with another galaxy. This disturbance could be responsible for the tidal features and irregular shape. 
