The object appears to be a single, luminous galaxy at a considerable distance, exhibiting a smooth, elliptical morphology. The galaxy presents a notable color gradient, shifting from a central region of enhanced yellow to a distinctly bluer outer halo. This suggests a differential stellar population distribution, potentially indicating older, redder stars concentrated towards the core, and younger, bluer stars in the galactic outskirts. The isophotes appear largely regular, without prominent tidal features or significant asymmetries, implying it is most likely not undergoing a major merger at the time. There is a mild suggestion of a minor asymmetry or disturbance. The light is centrally concentrated, although a faint diffuse envelope is present.
