The galaxy presents as an elliptical morphology, with a high degree of central concentration. There is a smooth, almost featureless appearance to the light distribution, with no apparent spiral arm structure. The color gradient suggests an older stellar population, shifting from a yellowish-white core to a slightly redder outer halo. The isophotes appear largely regular and elliptical in shape. There is a slight suggestion of possible tidal features or minor disturbance in the outer regions, but no distinct merging events are visible. The galaxy appears relatively isolated, with no obvious signs of close companions or major interactions.
