The galaxy presents as a relatively smooth, centrally concentrated elliptical morphology. The light profile appears generally featureless, exhibiting a radial gradient that brightens towards the galactic center. There is a hint of a color gradient, with the central region displaying a slightly redder hue compared to the outer regions which are more greenish-yellow. The galaxy does not exhibit any prominent spiral arms or a distinct disk structure based on visual assessment, nor any obvious signs of tidal disturbances or ongoing mergers, indicating it is most likely undisturbed. The morphology suggests an evolved stellar population.
