The galaxy presents as a slightly elongated, disk-like structure. The light distribution is concentrated towards the center, indicating a possible bulge or a bright nucleus, though not a perfectly circular disk, but more cigar-shaped. Its color appears relatively uniform across its extent, exhibiting a subtle gradient with a slightly bluer hue in the outer regions and a subtly redder appearance toward the central area. This suggests a degree of ongoing star formation, possibly more active towards the periphery. There is some evidence of minor disturbances in the light distribution, hinting at potential interactions or past merger events, but it appears largely unperturbed. There is also some visual smoothness to its structure. 
