The galaxy appears to be an elliptical, or possibly lenticular, galaxy. Its light is concentrated in a central bulge with a fairly smooth appearance. The concentration of light diminishes gradually from the center. There is only very faint visible structure, such as spiral arms or dust lanes, suggesting the galaxy is relatively evolved. The galaxy exhibits a yellowish-orange hue, indicating an older stellar population. It appears to be fairly isolated with no significant signs of recent or ongoing major mergers. The shape appears closer to round than cigar-shaped. There are no features to suggest a strong disturbance.
