The galaxy presents a generally smooth, elliptical morphology. The central bulge exhibits a concentrated luminosity, appearing yellowish-white, suggesting a population of older stars. Moving outward from the core, the light diminishes, creating a halo effect. The shape is generally in between being round, tending more towards being slightly elliptical. There is no obvious evidence of spiral arm structure or significant dust lanes. No major mergers appear to be occuring, but based on faint disturbances to the shape of the galaxy it may have had minor interactions. There are faint star forming properties.