The galaxy appears to be a relatively smooth, centrally concentrated object with an elliptical morphology. The light distribution suggests a high degree of symmetry and a lack of prominent spiral arms or distinct features. It is relatively round in shape. The central region exhibits a brighter, more intense yellow or orange hue, indicating a potentially older stellar population. Fainter blueish scattered light extends outwards in a slightly disturbed fashion from the object, particularly towards the top of the image. Overall, the galaxy presents as a relatively undisturbed system, without evidence of major mergers or strong tidal interactions based on its shape. However, the scattered light suggests that there is a small merger occurring.
