The galaxy presents a generally smooth and concentrated morphology, appearing largely spheroidal in shape. There is little evidence of spiral arm structures or a prominent disk. The light distribution is centrally concentrated, with a bright core region that fades gradually outwards. The galaxy is slightly elongated, but not significantly so. There appear to be no major disturbances, such as tidal tails or strong asymmetries, to suggest recent or ongoing major merger events. Subtle color variations are visible, with the central regions displaying a bluer hue compared to the outer halo.