The galaxy presents a somewhat elliptical morphology, exhibiting a core with a high surface brightness that appears nearly spherical from our vantage point. The central region transitions into a diffuse halo with a noticeably lower surface brightness. Subtle color variations are observed across the galaxy, hinting at varying stellar populations. The central region appears slightly more yellow in color compared to the outer halo. The halo appears to extend further along one axis, which could be due to a disk-like structure or tidal interactions. There is evidence of possible minor disturbances with a slight warping of the galaxy's structure. This might suggest a minor merger or interaction with a smaller companion.
