The galaxy presents as a spiral structure with a prominent central bulge. The arms appear relatively tightly wound, displaying a flocculent morphology. The bulge exhibits a smooth, concentrated luminosity profile. The disk is inclined at an intermediate angle relative to our line of sight. Evidence of a stellar bar structure crossing through the central bulge is present. The color distribution suggests a diverse stellar population, with bluer regions tracing spiral arms and a redder concentration toward the bulge.
