The galaxy presents as a flattened disk, viewed almost perfectly edge-on. It exhibits a prominent central bulge region that appears relatively smooth. The disk itself seems to be composed of stars and gas, however, minimal dust is evident. Faint blue hues can be observed at the outer edges of the disk. There is no visible evidence of a strong ongoing merger or tidal interactions, and there are no disturbances within the galaxy. The bulge appears to be rounded. The galaxy exhibits moderate luminosity. Star formation activity is either quite low or completely suppressed.