The galaxy appears to be undergoing a merger or strong interaction with at least one other galaxy. A primary, larger component displays a largely smooth, elliptical morphology, with a somewhat diffuse halo. The light distribution is concentrated in the central region, but not perfectly symmetrical. Adjacent to this component, another distinct galaxy is visible, presenting a more irregular shape. There are visible tidal tails, indicating strong gravitational interactions. The presence of faint red regions may indicate areas of intense star formation activity. The overall system exhibits an asymmetrical morphology, characteristic of disturbed systems, consistent with a galaxy merger.
