The galaxy presents as a luminous, elliptical system with a prominent central bulge. The core exhibits a high surface brightness, appearing nearly spherical and intensely bright. Radiating outward from the core, the galaxy displays a smooth, diffuse halo with a gradual decline in luminosity. This outer region is elongated, exhibiting a slight flattening along its periphery, indicative of a spheroid shape with some rotational influence. There is a subtle color gradient from the core to the outer halo, where colors become redder suggesting a change in stellar population. No distinct spiral arm structures or dust lanes are apparent. The overall morphology suggests an early-type galaxy, possibly an elliptical galaxy with minimal recent star formation activity.
