The galaxy presents as a largely featureless elliptical or lenticular galaxy with a smooth light distribution and a high degree of central concentration. The core exhibits a yellowish hue, which could indicate an older stellar population dominating the central regions. The outer regions appear slightly redder compared to the core, which might suggest a moderate amount of dust obscuration or color gradients associated with variations in stellar populations. There is no obvious spiral structure. The galaxy seems to be fairly isolated, lacking clear signs of any ongoing major mergers or tidal disturbances within the immediate vicinity.
