The galaxy appears to be an elliptical or lenticular type, exhibiting a smooth, centrally concentrated light distribution. The galaxy shows a bright, yellowish-white core, suggesting an older stellar population dominates the central regions. The outer regions show a more diffuse light, with some indication of a faint, extended halo. There are minor distortions evident in the outer parts of the disk. The overall shape appears somewhat elongated, with an apparent flattening. The disk appears to be nearly edge-on. There seems to be no clear presence of spiral arms or significant dust lanes. The galaxy displays a red-shift, indicating it is receding from us and is relatively distant.
