The galaxy presents as a centrally concentrated object with a largely smooth morphology. Its shape is generally elliptical, tending toward a slightly flattened spheroid. The galaxy's light distribution indicates a relatively evolved system, lacking prominent spiral arms or significant dust lanes.

There is faint color variation throughout, perhaps indicating differing stellar populations across its surface. The central region shows a subtle increase in luminosity, consistent with the presence of a galactic bulge. Possible minor disturbance can be detected in the shape of the galaxy, but this is small.
