The galaxy presents as a relatively smooth, centrally concentrated object, appearing elliptical in shape. The core exhibits a bright, yellowish-orange hue, possibly indicative of an older stellar population or significant dust obscuration. The outer regions display a gradual decline in surface brightness, fading into a more diffuse, bluish halo. There is minimal evidence of spiral arms or distinct features such as star-forming regions. The galaxy appears relatively undisturbed, lacking any obvious signs of major mergers or tidal distortions. Based on morphology, it is likely an elliptical galaxy, though a very face-on spiral galaxy cannot be entirely ruled out.
