The galaxy presents a primarily smooth morphology. The central region exhibits a high concentration of light, appearing nearly spherical and yellowish-white in color, suggesting an older stellar population. Fainter, bluer extensions surround this bright core, indicating the presence of some star formation. The overall shape appears largely undisturbed, although some subtle irregularities or features might exist within the surrounding disk. There are no clear signs of a major ongoing merger, though the galaxy appears to exhibit some minor disturbances within the galactic disk. The galaxy appears to be relatively round, showing minimal signs of distortion.
