The observed galaxy presents a predominantly smooth morphology. It exhibits a distinctly elongated, cigar-shaped structure, with a clear asymmetry along its major axis. While the galaxy generally lacks sharply defined features, there is evidence of minor disturbances in the galactic structure. The central region displays a slightly brighter, more concentrated luminosity, potentially indicating a bulge. Overall, the galaxy appears to be in a relatively stable state, with no signs of on-going major mergers or significant tidal interactions, though it's shape suggests some gravitational interactions in the past. The color gradient shows a possible transition from slightly redder colors at the ends of the galaxy to bluer colors in the central region, potentially indicating younger stars in the center or dust obscuring the ends.
