The galaxy presents a flattened, elliptical morphology with a high degree of central concentration. The light profile appears smooth, lacking any distinct spiral arm structures. The galaxy exhibits a strong, luminous core that gradually fades into the outer regions of the disk. Color gradients are subtle, with a slightly redder hue towards the center and a bluer tinge near the edges. The disk appears moderately inclined relative to our line of sight. There are no prominent signs of recent or ongoing major merger events. The overall visual impression suggests a relatively evolved system, possibly a lenticular or early-type spiral galaxy.