The galaxy presents a smooth, elliptical morphology. Its light is dominated by yellow and red wavelengths, suggesting an older stellar population. A slight elongation is observed, deviating from a perfect spherical shape. No distinct spiral arms or a prominent galactic disk are visible. There are no obvious signs of recent or ongoing major mergers or significant tidal disturbances in its structure. The galaxy's light profile appears relatively uniform, without intense concentrations of star formation. The overall impression is that of a mature, quiescent galaxy.
