This galaxy presents an overall elliptical morphology, although with some slight features suggesting a potential disk-like structure. The light distribution appears relatively smooth, with a central bulge that transitions into a fainter, more diffuse surrounding area. The color gradient shifts from a yellowish-white core to a faint greenish outer region, implying variations in stellar populations and possibly ongoing star formation within these outer regions. There is no indication of significant merging activity or tidal disturbances, suggesting that the galaxy is relatively undisturbed. The overall impression is that of a galaxy that is more elliptical in nature with some disk features present, indicative of older stellar populations dominating with some younger stars present in the outer regions.
