The galaxy presents as a centrally concentrated, smooth, and largely featureless elliptical galaxy, exhibiting a high degree of radial symmetry. Its light profile suggests a spheroid-dominated morphology with a relatively compact core.

The color gradient transitions smoothly from a yellowish-white core to a reddish-orange outer halo, possibly indicating an older stellar population throughout the galaxy. The absence of any notable dust lanes, spiral arms, or irregular structures suggests a well-mixed and relaxed system that has likely undergone significant dynamical evolution.

The galaxy appears to have a high degree of roundness. There is no evidence of any significant ongoing mergers or tidal interactions in the surrounding environment, and the galaxy displays a regular and symmetrical outer isophote shape.
