The galaxy presents a largely smooth, centrally concentrated morphology. Its overall shape appears elliptical, exhibiting a high degree of roundness with no obvious spiral arm structures or a pronounced disk. The light distribution is concentrated towards the center, which appears more luminous. There may be minor disturbances from other galaxies. Color gradients are subtle, with a hint of a redder core transitioning to slightly bluer outer regions. The galaxy's relatively compact size indicates it is likely a galaxy with moderate stellar mass and a low star formation rate.
