The galaxy presents as a relatively smooth, centrally concentrated object. Its overall morphology suggests an elliptical or lenticular galaxy. The core exhibits a bright, yellow-orange hue, potentially indicative of an older stellar population or significant dust content. Moving outwards, the light gradually fades into a more diffuse, blueish halo. There is no clear indication of spiral arms or a distinct disk structure. The galaxy appears mostly undisturbed, with no significant signs of tidal interactions or ongoing merger events. The shape appears largely rounded, lacking a strongly elongated or irregular form.
