The galaxy presents a generally smooth, elliptical morphology. Its color profile indicates an older stellar population, with a yellowish-orange hue dominating the central region. There is a subtle gradient in color, transitioning to a slightly redder outer halo. There is a hint of a disk structure, although indistinct, and no substantial evidence of spiral arms or significant star formation. Minor disturbances are present, but no major merging event is apparent. The galaxy appears to be relatively massive, with a weak rate of star formation. The shape is somewhere between round and elliptical. 
