The galaxy presents as a centrally concentrated object, elliptical in shape, with a smooth, diffuse light distribution and no readily apparent spiral arm structure. The core exhibits a bright, yellowish-white glow, suggesting an older stellar population or possible AGN activity. The surrounding halo fades outward, displaying a subtle color gradient from yellow/green transitioning to a darker redder outer region. This suggests a variation in stellar populations within the galaxy. There may be some minor tidal features, but the overall morphology does not suggest any major ongoing merger events. The galaxy appears largely undisturbed, exhibiting characteristics consistent with an elliptical galaxy that has undergone relatively little recent star formation.
