The galaxy presents as an elliptical morphology. Its structure is mostly smooth and centrally concentrated, showing a bright, yellowish core that likely signifies an older stellar population. Moving outward from the core, the light gradually diffuses, indicating a decline in stellar density. There is little evidence of spiral arms, dust lanes, or regions of active star formation; the overall color appears redder. It is slightly aspherical and more "in between" in shape, and is not interacting with any other galaxies.
