The galaxy appears as a centrally concentrated object, exhibiting a smooth, elliptical morphology. It is generally regular in shape, though a slight elongation is observed. The light profile appears consistent with a de Vaucouleurs profile. Color gradients are subtly present, trending toward bluer hues in the outer regions, which may indicate the presence of younger stellar populations at the edges. There is some evidence of minor disturbance in the form of faint tidal features or asymmetries which may suggest a past interaction or ongoing minor merger event, but this is not overtly noticeable.
