The galaxy presents as a disk galaxy, observed nearly edge-on from our vantage point. There is a clear central bulge which appears smoothly rounded. The disk is visible as a faint, elongated structure extending outwards from the bulge and the galaxy appears relatively undisturbed, exhibiting no strong signs of recent or ongoing major merger activity. The overall color suggests an older stellar population is dominant within the galaxy. This is supported by the smooth appearance and lack of pronounced spiral arm structure. The disk is thin and the galaxy exhibits a small amount of light in the blue band, indicating that there is very little star formation going on. The galaxy has a stellar mass on the order of 10^10 solar masses, and the lack of star formation within it suggests that it could be considered a red and dead galaxy.
