The galaxy appears as a relatively smooth, centrally concentrated object, exhibiting an elliptical morphology. The light distribution suggests a dominant spheroidal component. There are subtle color gradients; the central region appears slightly brighter and whiter, fading towards the edges. The overall texture is relatively smooth, indicating it is likely an older system with a lower ongoing star formation rate. The light emitted by the galaxy suggests its mass is high. The smooth appearance indicates it is unlikely to be undergoing a major merger. There appears to be an absence of distinct spiral arm structures or significant dust lanes. There are slight signs of minor disturbances. The shape appears more in between round and elliptical, leaning towards elliptical.
