The galaxy presents as a relatively smooth object with a slight central bulge. Its overall shape is generally elliptical, appearing mostly round. The galaxy exhibits a color gradient, transitioning from a reddish hue at its core to a bluish halo. There is no clear evidence of a distinct spiral structure or strong tidal features to suggest a recent major merger event. The light distribution is concentrated towards the center, which may point to a fairly old stellar population and low star formation rate. There is also a hint of a small disturbance.
