The galaxy presents an overall elliptical morphology, appearing largely smooth and concentrated. There is a suggestion of a central bulge region which is more intense and yellow in color. A faint, extended disk structure is also observed around this central concentration, with a bluer hue suggesting the presence of younger stellar populations. There may be very subtle indications of minor disturbances in the morphology. No spiral arm structure is readily apparent. The galaxy appears to have intermediate roundness.
