The galaxy appears to be undergoing a merger event. There is a primary, larger component which is relatively smooth in appearance with a concentrated, bright core. A smaller secondary component, roughly half the size of the primary, is visible offset to the west. There is evidence of tidal disruption, with faint, diffuse material extending outward, especially between the two components.

The primary component is somewhat rounded. The overall color of the system is yellowish-white, indicating an older stellar population with ongoing star formation. The estimated physical size of the primary component is approximately 5 kpc in radius.
