The galaxy presents a relatively smooth, elliptical morphology. It appears approximately round in shape. The light is concentrated in the center, with a radial decrease in brightness outwards. The color profile shifts subtly from a yellow-red core to a greenish hue in the outer regions, potentially indicating a change in stellar populations or dust distribution. There is no immediately apparent spiral structure or significant tidal disturbance suggesting a recent major merger event. The object appears to be an isolated galaxy.
