The galaxy presents as a luminous, centrally concentrated spheroid with a generally smooth appearance. The core exhibits a yellow-white hue, suggesting an older stellar population. The light from the central region gradually fades into a dimmer, extended halo. Hints of reddish tones are observable in the outer regions of the halo. There are no apparent spiral arms or significant dust lanes, indicating that the system is primarily composed of older stars with minimal ongoing star formation. Overall, the morphology is consistent with that of an elliptical galaxy at a moderate redshift.
