The galaxy presents as a largely featureless, elliptical or S0 morphology. Its light is dominated by a smooth, centrally concentrated bulge that emits strongly in the yellow-orange wavelengths, suggesting an older stellar population. The galaxy's overall form is generally round. There is a faint hint of a disk component or arm structure, but the image resolution limits a definitive classification.

While the galaxy appears relatively undisturbed, there may be faint tidal features or minor asymmetries indicative of past interactions. No clear signs of active merging are apparent. The galaxy exhibits a noticeable color gradient, transitioning from a yellowish core to a slightly bluer halo or outer regions, potentially indicating varying stellar populations or dust content.
