The galaxy presents as a single, relatively smooth object with a central concentration of light that gradually diminishes towards the outer edges. The overall morphology is elliptical in nature, with a high degree of circularity. There is little evidence of spiral arms or a well-defined disk structure. The galaxy's color gradient transitions from a yellowish-white core to a redder periphery. No distinct dust lanes or active star-forming regions are apparent. Faint disturbances are seen, indicating a potential past minor merger event, though the galaxy appears largely undisturbed at present.
