The galaxy presents as a relatively smooth, disk-like structure. It exhibits an elongated, cigar-like morphology. The central region is a bright, concentrated bulge with a noticeable yellow-orange hue, which may indicate an older stellar population. Fainter, bluer light is observed in the extended disk, hinting at ongoing star formation. There are no clear spiral arms or significant dust lanes visible in this image, but there seems to be a minor disturbance on the left side of the galaxy. There does not appear to be any neighboring galaxies or companion galaxies disrupting its shape. 
