The galaxy appears as a faint, diffuse structure with a slightly elongated morphology. There is evidence of a faint disk, though it seems somewhat disturbed or irregular. The color gradient suggests older stellar populations. The low surface brightness indicates that the galaxy is either relatively low mass or at a significant distance. The system does not appear to be undergoing a major merger, but there is the possibility of minor tidal disturbances. There is no prominent central bulge.
