The galaxy presents a generally smooth, elliptical morphology. Its light is concentrated towards the center with a gradual decrease in intensity outward. The object appears more rounded than elongated. There is no evidence of spiral arms or a prominent disk structure. Indications suggest that merging is not occurring. The color profile appears mostly uniform with a slight redder hue, which suggests older stellar populations. The galaxy is estimated to have a substantial mass, and is exhibiting low levels of star formation. 
