The galaxy presents as an elliptical or lenticular type, with a relatively smooth, featureless appearance. The central region exhibits a high concentration of light, suggesting a prominent bulge. Moving outwards, the light gradually decreases in intensity, showing a smooth transition from the core to the outer regions. There is an apparent lack of distinct spiral arm structures or significant dust lanes. The shape is moderately elliptical, appearing closer to round, but not perfectly spherical. Subtle distortions are possibly present, but these are not indicative of a major ongoing merger event. Colors appear generally redder, though subtle variations are seen within the galaxy. A faint blue halo may be present. The overall morphology suggests a galaxy with a dominant old stellar population. The star formation rate is relatively low.
