This galaxy appears to be a relatively smooth, isolated system exhibiting characteristics of an elliptical galaxy. The object demonstrates a notable central concentration of light, gradually decreasing in intensity towards the outer regions. A slight elongation is visible, with an apparent axis ratio close to 2:1.

Color gradients suggest a population of older stars. The galaxy is dominated by redder colors in the central region, shifting toward somewhat bluer colors in the outskirts.

There is a hint of morphological disturbance in the object, but a significant merger is not evident. There is no obvious disk, and it is unclear if there is any active star formation.