This galaxy presents as a system undergoing significant interaction or disturbance. The morphology does not appear to be a simple elliptical or spiral. There are several distinct light concentrations within the system. The primary concentration appears somewhat smooth, but is elongated and irregular in shape, possibly indicative of tidal forces at play. A second concentration appears more compact and distinct, and possibly a blueish hue. Overall, the light distribution is patchy, with several areas exhibiting a bluer color, suggesting regions of active star formation. There is no clear nucleus or disk structure visible. The relatively diffuse nature of the light, combined with the disturbed morphology, suggests that the galaxy is in a late stage of a merger, or has experienced a recent disruptive event.
