The galaxy presents as an elongated, cigar-shaped structure. Its light profile is dominated by a smooth, centrally concentrated bulge, appearing a reddish-orange hue suggesting an older stellar population. The overall morphology hints at an elliptical galaxy or a lenticular galaxy viewed edge-on. There is a subtle suggestion of a faint disk component. No strong spiral arm features or significant dust lanes are visible in this image, pointing towards relatively low levels of current star formation within the galaxy. The galaxy shows no obvious signs of a major ongoing merger, though some minor morphological disturbance cannot be ruled out.
