The galaxy presents a largely smooth and elliptical morphology. It displays a prominent central bulge that appears to be comprised of older stellar populations, as evidenced by its yellowish hue. The overall shape is somewhat elongated, appearing cigar-shaped, although it is mostly in between round and cigar-shaped. There is no obvious evidence of spiral arm structure or a well-defined disk component. The galaxy appears relatively isolated, with no clear signs of any ongoing major mergers or significant tidal disturbances. There is a hint of bluer color in the outskirts, possibly indicating some low-level star formation activity. This is consistent with a relatively massive galaxy that is gradually quenching its star formation.
