The galaxy presents as a relatively smooth, elliptical-like structure. Its color is predominantly yellowish-orange, suggesting an older stellar population with a lower rate of ongoing star formation. There is a slight hint of blue-green in the surrounding halo, perhaps suggesting the presence of a small population of younger, hotter stars. The galaxy does not exhibit any obvious signs of spiral arms or a prominent disk structure. No major mergers or disturbances can be seen, although there is a chance of a minor disturbance. The shape is generally round.