The galaxy presents a spiral morphology with a relatively bright central bulge. The disk component is well-defined, exhibiting distinct spiral arm structures. These arms appear to be tightly wound, tracing a complex pattern as they emanate from the central region. The overall color suggests a bluer stellar population, hinting at ongoing star formation processes within the galaxy. There is a lack of a significant bar structure apparent in the central region. While the galaxy appears relatively isolated, the morphology shows some degree of asymmetry, possibly indicating a minor gravitational interaction or recent accretion event. The light distribution suggests a smooth decline from the center outwards.
