The galaxy presents as a relatively small, smooth object. Its morphology appears to be predominantly elliptical. The light is generally homogenous, but a slight gradient in light intensity is visible as you travel from its center to the edges. Based on the slight colour variation, the light is composed of a range of wavelengths from the green, red and blue bands. The overall colour index suggests a stellar population that is relatively mature with a low ongoing rate of star formation. There is no apparent spiral structure or bar. There are some indications of minor disturbances. The galaxy is likely relatively low mass.
