The galaxy appears to be a relatively smooth object, with a slight elongation along its major axis. The light distribution suggests a concentration of older stars, as evidenced by the redder color in the central region. There is also a noticeable blue-green component, hinting at the presence of younger stars and potential ongoing star formation. The overall morphology is that of a somewhat disturbed system, potentially undergoing or having recently undergone a merger event. This is suggested by some asymmetry in the outer regions, as if there is an object disturbing it to the left.
