The galaxy presents a largely smooth and rounded morphology. The central region exhibits a bright, concentrated core, suggesting a significant stellar population and potentially a supermassive black hole. The color profile appears to be dominated by yellow and red hues, indicating an older stellar population with lower levels of ongoing star formation. There is little evidence of spiral arms or a prominent disk structure. Some faint diffuse light extends outwards from the core, forming a halo-like structure, although no distinct features like tidal tails or strong asymmetries are visible. Based on the appearance, it is likely an elliptical galaxy at a moderate redshift.
