The galaxy presents as a relatively smooth, centrally concentrated object. Its overall color appears slightly reddish. There is a subtle elongation, with an intermediate axis ratio. No distinct spiral arms or bar structure are discernible. There is very little, if any, apparent disturbance or interaction with other galaxies in the immediate vicinity. Based on its redshift, the galaxy is relatively distant. The relatively smooth morphology suggests that it is not undergoing a major merger event and the weak star formation rate indicates that it is likely a galaxy with more evolved stellar populations and less active star formation.
