The galaxy presents as a spiral type with a moderately bright central bulge. The disk component is visibly extended with well-defined spiral arm structures. The arms appear tightly wound, tracing a symmetric pattern around the galactic core. The color gradient suggests active star formation regions distributed throughout the spiral arms, with a bluer hue apparent. A relatively face-on orientation allows for a clear view of the disk morphology. There is a faint hint of a bar-like structure bisecting the bulge, although its exact form is not well-defined. No clear signs of major mergers or tidal disturbances are evident, giving the overall impression of a relatively undisturbed and mature spiral galaxy. The bulge exhibits a yellow color, indicative of an older stellar population.
