The galaxy presents as a centrally concentrated, elliptical-like structure. There's a distinct yellowish-orange core that diffuses outward into a fainter, more diffuse halo. The overall shape is roughly elliptical but appears somewhat perturbed, showing hints of non-smoothness. The outer regions exhibit a subtle blueish tint, possibly indicating some recent star formation activity. No clear spiral arms or disk-like structures are discernible, suggesting a lack of well-defined organized structure. The lack of strong morphological features may also point to an older stellar population dominating this system. There is a slight elongation, and the galaxy seems to have a somewhat moderate size relative to other background objects, fitting with a high mass estimation.