The galaxy presents an elliptical morphology with a central bulge that appears smooth in texture. The light distribution suggests that it is largely comprised of older stellar populations. There is a slight elongation to the shape. The disk component, if present, is not readily discernible. The overall color suggests a redder spectral energy distribution, consistent with a lack of significant ongoing star formation. There are slight disturbances, suggesting there may have been a minor merger, but not a major one.

The galaxy exhibits a luminosity suggesting a high mass. Star formation is expected to be low.