The galaxy presents as a relatively smooth, single structure. Its overall shape is somewhat elliptical, appearing mostly round, though not perfectly circular. There are no immediately obvious spiral arms or a prominent central bar visible. The galaxy exhibits a color gradient, with a bluer hue concentrated toward the center, transitioning to slightly redder tones in the outer regions. This may indicate a higher concentration of younger, hotter stars in the galaxy's core, and older, cooler stars toward the edges. There are no signs of major mergers or tidal disturbances, although there might be minor irregularities in its form. Overall, the light distribution is fairly concentrated, with no extended halo easily visible in this image.
