The galaxy presents as an elongated, disk-like structure with a prominent central bulge. The color gradient indicates an old stellar population. The central bulge exhibits a yellowish hue, suggestive of older, cooler stars. Moving outwards from the core, there is a subtle transition towards bluer colors in the outer regions of the disk, possibly indicating some ongoing star formation. The disk appears relatively smooth and symmetrical with no signs of major disturbances. The shape of the galaxy is cigar-shaped, the galaxy is quite elongated. There are no spiral arm structures visible.
