The galaxy presents as a single object with a relatively smooth morphology. The shape appears somewhat elliptical and is more in between round and cigar shaped, displaying a slight elongation. Its light is dominated by redder wavelengths. The galaxy exhibits a distinct core region with a high concentration of red light.  The outer regions display a gradient of decreasing intensity, fading into the background. This indicates a relatively low star formation rate. The structure shows no evidence of major disturbances or ongoing merging activity, though minor disturbances can not be ruled out. 
