The galaxy appears as an elongated, cigar-shaped structure, viewed at a considerable angle, possibly nearly edge-on. It exhibits a smooth, largely featureless morphology. The galaxy displays a subtle gradient in color across its length, suggesting variations in stellar population or dust content. There is a slight concentration of light towards the center, but no distinct nucleus is apparent. The galaxy appears relatively isolated, with no obvious signs of major interactions or mergers, although a minor disturbance cannot be ruled out. Its overall structure indicates it could be a lenticular galaxy, or possibly a spiral galaxy viewed edge-on with weak or obscured spiral arms. It has a blue hue, possibly indicating some low level of star formation.
