The galaxy appears to be a relatively compact elliptical galaxy, with a smooth, concentrated light distribution. Its core is bright and gradually fades outwards without exhibiting distinct spiral arm structures or prominent dust lanes. It is somewhat lenticular, with a slight elongation along its major axis. There is a subtle hint of a faint, extended halo surrounding the main body of the galaxy, with a slightly bluer color. Overall, the morphology suggests a relatively evolved system with a quiescent star formation rate. There are indications of minor gravitational disturbances in the symmetry of the outer halo.
