This galaxy exhibits a prominent disk structure, viewed at an oblique angle. Spiral arms are clearly visible, extending from a central bulge region. The arms appear somewhat loosely wound. The bulge displays a smooth, concentrated luminosity. The color distribution suggests active star formation regions within the spiral arms, contrasted by the yellower, older stellar population in the bulge. There is no apparent interaction with other galaxies or significant disturbances. A bar structure is not prominently visible within the central region.
