The galaxy presents as a relatively small, elliptical structure. The central region exhibits a pronounced brightness, suggesting a high concentration of stars or possible active galactic nucleus activity, although no distinct point source is resolved in this image. The isophotes appear generally smooth and regular. A faint, diffuse halo surrounds the brighter core, gradually fading into the background sky. There is evidence of some color variation, a subtle bluer color is noted on the outer edge of the galaxy. This suggests a small amount of younger star formation is occurring there. There is also evidence of a dark band in the central region of the galaxy.

Overall, the galaxy appears to be a relatively undisturbed system.
