The galaxy presents a generally smooth, elliptical morphology with a high degree of central concentration. Its overall color appears to be a pale yellow, suggesting a stellar population dominated by older, less massive stars. There is a slight color gradient visible, with the core appearing more yellow-white and the outer regions exhibiting a faint greenish tinge, potentially indicating the presence of some younger stars or ionized gas, though the star formation rate is relatively low. No prominent spiral arm structures or dust lanes are discernible, supporting its classification as an elliptical galaxy. There are also no obvious signs of major mergers or tidal disturbances, suggesting a relatively quiescent evolutionary history. The galaxy appears fairly isolated in this field.
