The galaxy presents as a relatively smooth and rounded object. There may be signs of a minor disturbance due to a merger event. There is not enough morphological information to determine the structure of any galactic disk. The galaxy has a slight inclination to our line of sight, as it appears round rather than elongated. Light from the galaxy appears with color in the green, red, and z bands. The luminosity indicates a galaxy of significant mass. The low star formation rate indicates it is not actively producing large numbers of new stars.
