The galaxy appears to be a relatively smooth, centrally concentrated system. Its light profile suggests an elliptical morphology or a lenticular galaxy seen face-on. The galaxy exhibits a slight color gradient, appearing bluer towards the center and becoming redder in the outer regions. This could indicate ongoing or recent star formation concentrated in the core, or a difference in the stellar populations, with younger, bluer stars dominating the central region. There is no obvious spiral structure, bar, or signs of active merging, although there is some slight asymmetric distortion. Overall, the galaxy seems relatively undisturbed and evolved.
