This galaxy appears to be an elliptical galaxy with a relatively smooth morphology. The light distribution is centrally concentrated, with the highest intensity light in the yellow/white spectrum. There is little evidence of spiral arms or significant dust lanes. The shape is generally round. No major merger events are visible, though a minor disturbance or possible interaction with a smaller companion galaxy cannot be ruled out based on the image. The galaxy seems to have a lack of active star formation and is composed primarily of older stellar populations.
