The galaxy presents as a relatively compact, elliptical-like system. Its overall color appears to be redder, indicating a population of older stars and a lower rate of current star formation. The light is centrally concentrated with a smooth profile. There is some subtle asymmetry and potential for minor disturbances in its morphology. There is no distinct spiral arm structure visible, which suggests this is not a typical spiral galaxy. The galaxy displays a fairly round morphology, and the low amounts of blue light observed from the galaxy indicates low ongoing star formation and likely older stellar populations.
