The galaxy presents as a largely smooth, round object with a concentrated central region. Its color profile indicates an older stellar population. The galaxy exhibits a gradient from a bright, yellowish core towards fainter, bluish outer regions, suggesting some presence of younger stars, but not a significant amount. No prominent spiral arms, bar structures, or dust lanes are discernible. The general morphology suggests an elliptical galaxy with a high degree of central concentration and a relatively uniform stellar distribution. There is no obvious sign of active galactic nucleus activity or significant star formation. The overall appearance implies a quiescent state.