The object appears to be a galaxy with a relatively smooth, elliptical morphology. The light distribution suggests that it is highly concentrated, with a bright core that fades outwards into a less luminous halo. There is a slight elongation, but overall the galaxy presents as largely rounded. Its color index suggests that the galaxy is comprised of an older stellar population, with lower levels of current star formation and potentially higher levels of dust absorption. The overall appearance of the galaxy suggests it is not undergoing any major mergers or disturbances. 
