The galaxy appears as a generally smooth, centrally concentrated object with a diffuse morphology. There is a noticeable radial gradient in surface brightness, with the central region exhibiting higher luminosity. The galaxy displays an ellipsoidal shape with a high degree of roundness, showing only slight deviations from a perfect circle. The galaxy's light distribution suggests a relatively homogenous stellar population, with no apparent distinct structural features such as spiral arms or a prominent bar. There are some subtle hints of possible disturbances or minor asymmetries in the outer regions, but the overall appearance is that of a well-formed galaxy. The color profile suggests a dominant older stellar population, and the faintness suggests it is far away. 
