The galaxy exhibits a generally spheroid morphology. The light profile is relatively smooth and concentrated towards the center, suggesting a dominant bulge component. There is little evidence of spiral arm structure or a well-defined disk. The galaxy's color is markedly blue, indicating active star formation or a younger stellar population. There is no clear tidal features or distorted morphology that would suggest a recent major merger event, but there is a slight elongation, suggesting a minor disturbance could be occuring.