The galaxy presents a smooth, elliptical morphology with a concentrated central bulge. The core exhibits a reddish-orange hue, possibly indicative of an older stellar population. A less concentrated, greenish colored halo surrounds the core of the galaxy, this coloration is indicative of ongoing, lower levels of star formation. Overall, the galaxy appears relatively undisturbed, exhibiting no signs of major merging activity or significant tidal features, and possesses a rather high degree of overall circularity.
