The galaxy presents as a luminous, elliptical structure. The central bulge exhibits a yellowish hue, suggesting an older stellar population, while the outer regions appear slightly bluer. The galaxy appears mostly smooth, with no obvious signs of strong spiral arms or a prominent disk. The object's shape is moderately elongated. There are no obvious signs of major tidal disturbances or ongoing merger activity, however, there are subtle suggestions of minor perturbations in its structure. It has a noticeable stellar formation which is not extreme, suggesting a moderate rate of star formation.
