The galaxy presents as a centrally concentrated luminous object. Its morphology appears predominantly smooth, with a high degree of circular symmetry in its overall shape. There is no apparent disk structure or indication of spiral arms. The galaxy exhibits a color gradient, transitioning from a brighter, more yellow-white core to a slightly fainter and redder halo region. No significant signs of ongoing mergers or tidal disturbances are visible in the immediate vicinity of the galaxy. It is likely an early-type galaxy with a considerable stellar mass and suppressed star formation.