The galaxy presents as a single, relatively smooth object with a bright central concentration. There is a noticeable color gradient from the center outward. The core appears to be composed of primarily older stars as evidenced by its yellowish-orange hue. Proceeding towards the edge of the galactic center, a small blue-ish or possibly green-ish tint can be seen. This suggests a presence of younger stars, though not nearly as much as in other galaxies, and low levels of on-going star formation. The shape is primarily elliptical. There appears to be no significant tidal disruption or other disturbances that would suggest a major merging event. Faint arm structure may be present, though these are not highly pronounced. Overall, the galaxy is fairly compact with a high degree of central concentration.
