The galaxy presents a generally smooth morphology, exhibiting minimal discernible features such as spiral arms or a prominent bar. It appears largely elliptical or spheroidal in shape, with a relatively high degree of roundness. A color gradient is observed, with a yellowish-white central region gradually transitioning to a bluish-white periphery. This suggests a concentration of older stellar populations in the core, and potentially younger, bluer stars in the outer regions, though active star formation is not strongly indicated visually. There is no apparent ongoing major merging activity, although a slight irregularity in the outer halo might suggest a minor interaction or past merger event. Overall, the galaxy appears to be a relatively evolved system.
