The galaxy presents as a centrally concentrated, ellipsoidal structure with a smooth light distribution. The core exhibits a yellow-orange hue, suggesting an older stellar population. The overall shape is primarily elliptical, with a high degree of central concentration and very little discernible substructure or spiral arm features. There is a slight elongation, but the galaxy is mostly circular in projection. The lack of defined features indicates a passively evolving system, possibly a lenticular or elliptical galaxy with minimal ongoing star formation. The galaxy shows no evidence of tidal disturbances or ongoing merger activity in this image.
