The galaxy presents a largely smooth, elliptical morphology. It is centrally concentrated with a gradual decrease in luminosity moving outwards from the core. The overall shape appears neither perfectly spherical nor significantly elongated, instead, the structure is somewhere in between the two. The lack of strong, well-defined features such as spiral arms or a distinct central bar suggests a relatively quiescent galactic environment. There might be minor disturbances in the outer regions of the galaxy, but no major merger events are evident from the image alone. The galaxy exhibits a color gradient, with the central regions appearing slightly bluer and the outer regions trending towards redder hues, which could imply a difference in stellar populations and star formation rates between the core and the outskirts.
