The galaxy presents as a disk galaxy observed nearly edge-on. A prominent central bulge is apparent, displaying a smooth, rounded morphology with a high concentration of light. The disk itself appears thin and elongated, with a suggestion of dust lane obscuration running along the equatorial plane of the galaxy, contributing to its reddish hue. There are no immediately obvious signs of major tidal disturbances or ongoing mergers, though the overall faintness of the disk structure makes identifying subtle features challenging. It is likely a relatively massive galaxy with ongoing, but not particularly vigorous, star formation.
