The galaxy appears as a somewhat elongated, lenticular-shaped structure. It exhibits a smooth, diffuse morphology with a brighter central bulge, possibly an elliptical galaxy viewed at an angle. The color profile indicates a subtle bluer hue in the outer regions compared to the yellower core. No distinct spiral arms or prominent dust lanes are discernible from this image. There are hints of minor disturbances present in the disk, but no signs of ongoing major merger events.