The galaxy presents a primarily smooth and elliptical morphology. It appears largely featureless, lacking any prominent spiral arms or a distinct central bar. Its shape is very close to round, with only a slight deviation towards an elongated form. The galaxy emits predominantly in the redder wavelengths, suggestive of an older stellar population. There is no indication of significant ongoing mergers or major disturbances. The light is diffuse and evenly distributed across the galaxy.
