The galaxy appears as a centrally concentrated, smooth object with a relatively high degree of symmetry. Its light profile suggests a gradual decline in surface brightness from the core outwards. There is no obvious spiral arm structure or bar feature. The overall color is somewhat blue, but not intensely so, suggesting intermediate stellar populations. There are no obvious signs of major mergers or tidal disturbances in the immediate vicinity, although a slight asymmetry in the outer regions cannot be ruled out without further analysis. The roundness of the galaxy is somewhere in between round and elliptical, leaning more towards the elliptical side.
