The galaxy presents a somewhat amorphous structure, appearing mostly smooth in its overall light distribution. It exhibits a shape that leans toward being intermediate in roundness, not perfectly circular but also not significantly elongated. There is faint evidence of some kind of disturbance in its structure, although major mergers are not obvious. There is faint blue light distributed throughout, suggesting recent star formation. The galaxy appears to be of intermediate mass and star formation rate, although it is still relatively inactive.
