The object under examination presents as a galaxy with an overall oblong morphology. The central region exhibits high luminosity, appearing nearly saturated in this observation. Surrounding the core, a flattened structure can be discerned. This structure, with a radial extent of approximately 8 arcseconds, suggests a possible disk-like component to the galaxy, though the resolution is insufficient to definitively classify it. 

There are some hints of disturbances within the galaxy. The outer regions of the object are more amorphous, displaying faint tendrils or asymmetries that depart from a smooth, elliptical profile. There is a hint of blue color within the inner regions of the galaxy. The overall color of the galaxy is slightly on the red side. This could be due to the age of the stars, amount of dust, or a combination of the two.
