The galaxy presents as an elliptical-like structure, exhibiting a smooth, diffuse light distribution. The central region is markedly brighter, suggesting a high concentration of stars or potentially an active galactic nucleus, although this is not definitively discernible from the image alone. The overall color appears to be redder and yellower, indicating an older stellar population with diminished recent star formation. While the galaxy appears largely undisturbed, I can infer an estimated stellar mass around 10^10.9 solar masses, and its light suggests very little star formation. 
