This galaxy exhibits a notable degree of smoothness in its overall morphology. While not a perfectly elliptical structure, the light distribution appears largely uniform, with the brightest region concentrated towards the core.

There is evidence of some disk-like structure present, as the galaxy appears somewhat flattened when viewed edge on. A faint blue region can be seen at one end of the galaxy, suggesting some degree of active star formation. It cannot be ruled out that there may be low-level merger activity going on. 

Based on its moderate redshift, this galaxy is at a considerable distance. Despite this distance, it still appears relatively luminous.
