The galaxy presents as two distinct components: one, a relatively bright, rounded structure with a smooth appearance; and the other, a more diffuse and elongated feature exhibiting signs of disturbance. The brighter, smoother component appears predominantly featureless with a generally circular morphology. The second, fainter component displays a distinctly disturbed morphology, with evidence of tidal features or possible interaction. There is an indication of active star formation within at least one of the components, inferred from a bluish tint. This object could potentially be undergoing a minor merger or experiencing some form of gravitational interaction with a nearby companion. The overall light distribution is relatively concentrated, suggesting a moderate degree of central mass concentration within at least the brighter component.
