The galaxy presents a distinctly elongated, cigar-shaped morphology. Its color profile indicates a dominant population of older stars, exhibiting a yellow-red hue, particularly concentrated within its central bulge. There is a subtle blue shift in color as you move toward the edges of the galaxy, potentially indicating the presence of younger stars or star forming regions along the disk. There is no distinctive spiral arm structures. The galaxy appears relatively undisturbed, showing no obvious signs of recent major merger activity. The morphology suggests the galaxy could be a lenticular galaxy with minimal star formation or an elliptical galaxy. Overall the galaxy appears to be a relatively massive system.
