This galaxy presents as an edge-on disk galaxy. There is a noticeable central bulge with a high degree of symmetry and a slightly boxy shape. The bulge appears luminous with a golden hue, indicating an older stellar population. A faint disk extends outwards from the central bulge on either side. The disk's dust lane is difficult to distinguish, but the disk appears narrow and relatively uniform in color, suggesting a lack of significant recent star formation. There are no obvious signs of active galactic nuclei activity or major mergers, although there are subtle irregularities in the disk, possibly indicating minor disturbances or tidal interactions. The galaxy appears to be fairly isolated.
