The galaxy presents a generally smooth, elliptical morphology. There is little discernible disk structure, and no clear spiral arms. The shape tends toward round, with only a slight deviation toward an elongated form. There are no indications of major mergers or significant tidal disturbances in the immediate vicinity. Color gradients are subtle, indicating a relatively uniform stellar population. The galaxy appears to be generally quiescent, with a low star formation rate, as suggested by the lack of bright blue regions that indicate active star formation.
