The galaxy presents as a moderately luminous, elliptical system at a redshift of approximately 0.2. The light profile appears smooth, with a high degree of central concentration and no discernible spiral arms or disk-like features. The isophotes are generally round, with a minor deviation towards a slightly elongated shape. The galaxy exhibits a subtle color gradient, appearing bluer towards the center and redder in the outer regions, suggesting a mixed stellar population with a possible younger component in the core. There is no evidence of significant dust extinction or active star formation. There are no signs of tidal disturbances or ongoing mergers.