The galaxy presents an overall elliptical morphology with a smooth, diffuse appearance. The main body of the galaxy exhibits a central concentration of light, gradually fading towards the edges. There is evidence of a slight elongation, indicating a deviation from a perfectly spherical shape. A subtle bluish hue is observed in certain regions, suggestive of the presence of younger stellar populations or ongoing star formation. Additionally, the presence of some form of disturbance cannot be ruled out with several regions of the galaxy showing more activity, especially on the left side. 
