The galaxy presents as an elliptical morphology, with a high degree of central concentration. The light distribution is smooth and centrally peaked, suggesting an older stellar population. It appears moderately elongated. The galaxy exhibits a color gradient, transitioning from a yellow-white core to a slightly bluer outer region. There is no apparent spiral structure or dust lanes. No major disturbances or signs of a merger are visible. The color and smooth morphology are consistent with a galaxy undergoing modest star formation.
