This galaxy exhibits a relatively smooth morphology, with a dominant central bulge. The galaxy appears nearly circular in shape, with no obvious strong spiral arm structures or a pronounced bar. There is a slight flattening to the structure of the galaxy. The color gradient suggests a higher concentration of older stars within the central bulge, while bluer hues may indicate the presence of younger stars in the surrounding disk. Faint extensions and distortions are visible surrounding the main galactic body, hinting at possible tidal interactions, which are not significantly disrupting the structure. No prominent dust lanes are obviously visible across the disk.
