The galaxy presents as a somewhat elongated, elliptical structure with a smooth light distribution. There is a centrally concentrated region exhibiting a yellowish-white hue, potentially indicative of an older stellar population. Surrounding this core is a larger, diffuse halo of greenish light. The green color suggests ongoing or recent star formation activity within the galaxy. The lack of well-defined spiral arms or a prominent disk-like structure supports its classification as an elliptical galaxy. There is no apparent sign of any major ongoing merger activity or significant tidal disturbances.
