The galaxy presents as a generally smooth, elliptical structure with a high degree of central concentration. The light distribution appears largely uniform, lacking prominent spiral arms or distinct features. The overall shape is somewhat elongated, exhibiting a slight departure from a perfectly circular morphology. A gradual decrease in luminosity is observed from the bright core outwards towards the periphery of the galaxy. There is faint color variation, where the central bulge appears to be composed of older stellar populations based on the redder color, and the outer disc appears more blueish, hinting at ongoing star formation. The galaxy does not show obvious signs of a major ongoing merger or significant tidal disturbances.
