The galaxy presents as a centrally concentrated, relatively smooth elliptical system. The core exhibits a bright, yellowish-white hue, suggesting an older stellar population. The outer regions of the galaxy fade gradually, showing a slightly redder tint than the core which suggests a continuation of older stars. The system displays a generally round morphology, with no apparent spiral arm structure or significant dust lanes. Overall, the galaxy appears to be a quiescent system with characteristics consistent with a well-formed elliptical galaxy. There are hints of a minor disturbance.
