The galaxy presents as a complex system, potentially undergoing a merger event or exhibiting signs of tidal interaction. It is comprised of two distinct luminous components. The first, located in the upper-right, appears as a relatively smooth, centrally concentrated spheroid, exhibiting a bright, yellowish-white core. The second component, found in the lower-left, shows a more irregular morphology with a distinct yellowish hue. There is some evidence of diffuse light extending between these two primary components, hinting at a possible tidal bridge or shared envelope. The overall shape deviates significantly from a simple elliptical or spiral structure, suggesting gravitational disturbance. Color variations suggest differing stellar populations or dust content within the system. The system seems to be quite evolved with a relatively low star formation rate.
