The galaxy presents a primarily smooth, elliptical morphology. It exhibits a concentrated central bulge that graduates outward into a more diffuse halo. The core region appears bright with an apparent yellow-white color, possibly indicating an older stellar population. The outer regions display a bluer hue compared to the core, suggesting the presence of younger stars. The galaxy appears well-defined, showing no signs of significant tidal disturbances or ongoing mergers. Overall, the observed light distribution supports a classification as an elliptical galaxy with a relatively high degree of symmetry.
