The galaxy presents a somewhat smooth, elliptical morphology. There is a bright central bulge that appears spheroidal with decreasing luminosity moving outwards. The disk component displays a diffuse and relatively even distribution of light, with a noticeable lack of prominent spiral arm structures. There is a slight indication of a disk, as the galaxy does not appear to be perfectly circular. The overall color profile suggests a higher concentration of older stellar populations. Very subtle disturbances may be present, but the galaxy appears relatively relaxed and undisturbed.
