The galaxy presents as a luminous elliptical type, exhibiting a smooth, centrally concentrated morphology. The light profile appears consistent with a de Vaucouleurs profile, showing a gradual decrease in surface brightness from the core outward. The core itself is bright and yellow, suggesting an older stellar population dominated by evolved giant stars. There is a subtle color gradient, with bluer tints observed in the outer regions of the galaxy. No prominent spiral arm structures or dust lanes are discernible. The galaxy appears relatively undisturbed, with no indications of major mergers or significant tidal interactions. The object presents as a large galaxy exhibiting an estimated stellar mass of approximately 10^10.8 solar masses. The rate of star formation is modest, with a specific star formation rate of approximately 10^-10.8 per year.
