The galaxy presents an elliptical morphology, exhibiting a smooth, centrally concentrated light profile. Its shape appears to be somewhat elongated, deviating slightly from a perfect sphere. A bright, yellowish core is clearly visible, suggesting a concentration of older stellar populations in the galactic nucleus. Surrounding this core is a more diffuse, bluish halo. This suggests the presence of a population of younger, bluer stars, although their contribution appears secondary to the yellow light from the core. The lack of well-defined spiral arms or dust lanes supports its classification as an elliptical galaxy. No significant signs of ongoing mergers or tidal disturbances are apparent.
