The galaxy appears to be an elongated, cigar-shaped object, likely an elliptical galaxy viewed at an oblique angle or possibly a highly inclined spiral. The light distribution is relatively smooth, with a concentrated central bulge that fades gradually toward the outer edges. A slight color gradient is noticeable, shifting from a more reddish hue in the center to a subtly bluer tint on the edges. It appears that there is little to no presence of active star formation withing the galaxy. There are no distinct spiral arms or obvious dust lanes visible. The overall structure suggests a relatively old stellar population within a galaxy that has undergone minor if any disturbances in the recent past.
