The galaxy presents as a relatively smooth, elliptical structure. Its morphology is dominated by a bulge with no discernible disk component. There is a bright central region, potentially indicative of an active galactic nucleus or a dense concentration of stars. The color appears to be generally yellow/orange, suggesting an older stellar population with relatively low ongoing star formation. There is no evidence of spiral arms, bar structures, or major disturbances indicative of recent or ongoing merger events. The galaxy exhibits a high degree of roundness with an overall symmetrical shape. There is a slight gradient in luminosity from the center outwards, indicating a decrease in stellar density with increasing distance from the core.
