The galaxy presents as a relatively compact, elliptical structure, exhibiting a high degree of smoothness and roundness. There is no discernible spiral arm structure or bar. The light is concentrated in the center. The color of the galaxy is generally consistent with an older stellar population. There is no strong evidence of recent major merger activity. The galaxy does not appear to be highly actively star-forming based on the smoothness and redder color. Small disturbances in the outer regions of the galaxy are barely detectable and appear very weak.
