The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that graduates into a more diffuse outer halo. The core region appears yellowish-white, indicative of an older stellar population. The color of the object reddens toward the center suggesting a higher concentration of older stars. A slight, almost imperceptible extension or distortion is present indicating a possible recent interaction or a subtle inherent asymmetry. No prominent spiral arms or dust lanes are discernible. Based on the lack of significant blue light, star formation appears to be relatively quiescent within this galaxy.
