The galaxy presents as a relatively smooth, lenticular system. It has an elongated shape, appearing mostly rounded although not perfectly spherical. The central bulge is bright and concentrated, exhibiting a somewhat yellowish-white color, suggesting an older stellar population. Surrounding the bulge is a fainter, more diffuse disk. The disk displays a subtle blueish tint, potentially indicating the presence of some younger, hotter stars, although current star formation is minimal. There are no prominent spiral arms or dust lanes visible. There are no indications of a major ongoing merger or significant tidal disturbances. There is possibly a minor disturbance present.
