The galaxy presents as a centrally concentrated, elliptical-type system. Its overall color appears to be yellowish-white, suggestive of a population of older stars with lower rates of on-going star formation. The galaxy exhibits a high degree of smoothness, lacking prominent spiral arms or distinct morphological features often associated with younger stellar populations. There is a slight elongation, indicating that the galaxy is not perfectly spherical, but rather somewhat flattened. Upon closer inspection, some faint peripheral light is visible surrounding the core, which suggests an extended halo component. Overall, the galaxy appears to be a relatively quiescent, evolved system.