The galaxy presents as a relatively smooth, elliptical object with a concentrated central bulge. The color profile appears generally redder, with a slight gradient toward the center. The shape is close to elliptical but not perfectly round, possibly hinting at a slight elongation or distortion. There is a very faint, diffuse halo surrounding the central region, suggesting a gradual decrease in stellar density with increasing distance from the core. The galaxy exhibits a relatively high Sersic index, indicating a steep concentration of light towards the center. Overall, the morphology suggests an evolved system with a predominantly old stellar population and minimal ongoing star formation.
