The galaxy appears to be a spiral galaxy viewed at a shallow angle, nearly face-on. It exhibits a prominent central bulge that diminishes in luminosity towards its edges. Evident are spiral arm structures, rather distinct as they extend from the core region. The arms are somewhat tightly wound, implying a more ordered structure. Within these spiral arms, we observe indications of star formation regions, distinguished by their bluer color. Dust lanes may be present, but the resolution limits confirmative identification. The overall color suggests a late-type spiral, but the lack of defined HII regions and tight spiral arm structure could signal a more passive star formation rate. The absence of any strong signs of tidal disturbance suggest it hasn't experienced a recent major merger. Based on its morphology, the galactic bar may be present but no very strong. The absence of significant blue color extending from the central bulge also implies minimal star formation activity in that region. The galaxy shows a moderate size.
