The galaxy presents as an elliptical morphology, exhibiting a smooth, centrally concentrated luminosity profile. The core appears yellowish-orange suggesting an older stellar population. Fainter extensions of light are visible, creating a slight elongation along one axis. There is no clear evidence of spiral arm structure or active star-forming regions. The overall structure appears relatively undisturbed, with no obvious signs of major recent mergers, although some minor disturbance cannot be ruled out at this resolution.
