The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a generally elliptical morphology, with no obvious spiral arm structure or strong irregularities. The central region displays a distinct yellowish-orange hue, suggesting an older stellar population, potentially dominated by evolved stars. This core region appears more compact and brighter than the surrounding halo. The outer regions of the galaxy are characterized by a fainter, more diffuse, and slightly bluer halo. There is no clear indication of any significant ongoing merger activity or major tidal disturbances in this image. The overall appearance suggests a galaxy that is relatively undisturbed and potentially nearing the end of its major star-forming phase.
