The galaxy presents a largely smooth morphology, appearing approximately elliptical in shape. There is a concentration of light towards the center, suggesting a bright galactic nucleus. The overall color appears yellowish, which could indicate an older stellar population with relatively low ongoing star formation. Irregularities and disturbances are suggested in the structure, potentially indicative of recent or ongoing gravitational interactions with other galaxies. A complex merger event is likely to have taken place recently in the galaxy's history. The galaxy may have a substantial mass given its morphology and coloration.
