The galaxy presents as a smooth, centrally concentrated object, with a relatively high degree of circularity. The light distribution appears largely homogenous, indicative of an elliptical or S0 morphology. There is a hint of a color gradient, the core slightly more yellow/red, suggesting an older stellar population centrally, and possibly bluer on the outer edge of the galaxy. The galaxy may be interacting with the other object shown, possibly another galaxy. This could explain the slight disturbances in the light, although a lack of defined tidal tails or bridges suggests the interaction is early.
