The galaxy presents as a centrally concentrated system, exhibiting a generally smooth morphology. The light profile appears elliptical, with a notable elongation. The core region displays a higher surface brightness, transitioning to a fainter, more diffuse halo.  Color gradients are subtle but present, with the central region exhibiting a slightly redder hue compared to the bluer outer regions, potentially indicating differing stellar populations or dust content. There is no discernible spiral arm structure or obvious signs of recent major mergers, though a slight asymmetry cannot be ruled out.  The lack of significant features suggests a relatively undisturbed evolutionary history.
