The galaxy presents as a smooth, elliptical morphology, with a high degree of central concentration. There is a noticeable lack of distinct spiral arms or disk-like structures. The light distribution appears mostly homogenous, indicating a relatively uniform stellar population. The galaxy exhibits an intermediate roundness. Faint extensions are visible, but no major disturbances indicative of ongoing mergers are detected. Color gradients reveal a generally yellow-reddish central region, which is typical for older stellar populations. A bluer component is observed in the outer regions, consistent with the presence of some younger stars or star forming regions. Overall, this galaxy is most likely an elliptical galaxy with an estimated mass of 10^9.7 solar masses and suppressed star formation.
