The galaxy appears to be a relatively smooth, disk-like structure with a hint of a central bulge. Its overall shape can be described as moderately elliptical. There's a color gradient observed, shifting from a bluer hue at the periphery of the disk to a redder, more yellow-toned central region. This may indicate differing stellar populations and star formation rates across the galaxy, with older stars residing in the core. There is little evidence of major spiral arm structure or significant dust lanes visible in this image, giving the galaxy a more uniform appearance. Subtle irregularities and asymmetries can be noted, possibly indicating minor past or ongoing interactions with other galaxies or internal processes affecting its morphology.
