The galaxy presents as a relatively smooth, elliptical structure, exhibiting a concentrated central bulge that fades gradually into a more diffuse halo. The core appears bright and yellowish, suggesting an older stellar population. Moving outwards, the overall color shifts slightly, with subtle hints of redder and bluer regions, particularly towards the edges of the halo, potentially indicating areas with some ongoing or recent star formation. The galaxy appears to have a high degree of rotational symmetry, with a slight elongation that gives it an oval shape. There is no strong evidence of spiral arms or significant dust lanes. There is also no indication of any major mergers or tidal disturbances that may have affected the morphology. Overall, the galaxy seems to be an elliptical galaxy in a relatively undisturbed state.
