The galaxy presents as an elliptical morphology, characterized by a smooth, diffuse light distribution with no readily discernible spiral arms or distinct features. The core is significantly brighter and more concentrated than the outer regions, indicating a likely concentration of stars and possibly a supermassive black hole at the galactic center. The galaxy exhibits a slightly elongated shape, suggesting a mild degree of flattening. The color profile appears relatively uniform, trending toward redder wavelengths, indicative of an older stellar population and subdued recent star formation activity. There might be slight evidence of tidal disturbances or interactions, with some faint asymmetrical features that could indicate past minor mergers. The overall appearance is consistent with a mature elliptical galaxy at a moderate redshift.