The galaxy presents as a generally smooth, elliptical-like structure with a concentrated central bulge. The light distribution appears fairly even across the galaxy, with a gradual fading toward the edges. There is a subtle redder hue in the central regions suggesting an older stellar population is centrally concentrated. There is evidence of a faint disk-like component, though it's not sharply defined and appears largely smooth. Slight disturbances may be present in the form of minor asymmetries in the outer regions, but the overall structure is relatively undisturbed. The galaxy exhibits a yellowish-white color, indicating a mixture of stellar populations. The roundness index is not entirely circular.
