The galaxy presents as a somewhat elongated, though primarily amorphous, structure. Its light profile appears centrally concentrated with a smooth falloff in surface brightness towards the outer regions. The color gradient transitions from a yellowish-white core to redder, more diffuse edges. There is a subtle indication of a possible disk-like component that is slightly disturbed or irregular. Overall the galaxy does not seem to be undergoing a major merger event, however, there may be a minor disturbance in its galactic structure.
