The galaxy appears as a centrally concentrated object with a generally smooth morphology. There is a slight elongation to the galaxy’s shape, giving it an appearance that is not perfectly circular. The color profile suggests a population of older stars, but the presence of some light in the bluer wavelengths indicates that there may be modest ongoing star formation within the galaxy. There are no strong indications of spiral arms or other distinct features, like rings. This suggests the galaxy is either an elliptical galaxy or a lenticular galaxy viewed at an angle where any disk-like structure is not apparent. There do not appear to be any strong signs of ongoing major mergers or tidal disturbances in this image, though some minor asymmetry cannot be ruled out.
