The galaxy presents as a generally smooth, elliptical form, though not perfectly rounded. It appears to be relatively undisturbed, with no obvious signs of major mergers or significant tidal disruptions in its immediate vicinity. There is a suggestion of some internal structure, but it is not strongly defined; there are slight color variations that may indicate regions of differing stellar populations or dust distribution, but these features are subtle. Overall, the galaxy exhibits a fairly quiescent morphology, lacking prominent spiral arms or a highly active nucleus. Its color suggests a galaxy with a relatively old stellar population and low ongoing star formation.
