The observed galaxy appears to be a spiral galaxy, viewed at a moderate inclination. The central bulge is relatively small and unresolved, suggesting a lower mass concentration in the core region. The disk component exhibits a mottled texture with a mix of bluer and slightly redder regions, consistent with ongoing star formation. There may be faint, loosely wound spiral arm structures, though they are somewhat indistinct. The overall shape appears relatively undisturbed, with no obvious signs of a major merger event, although there is some asymmetry. The galaxy has a noticeable blue tint in its outer regions, which is indicative of younger stellar populations and active star formation.
