The galaxy presents as a well-defined disk galaxy, likely a spiral galaxy, observed nearly edge-on. A central bulge component is visible as a concentrated region of brighter, yellowish light, indicative of an older stellar population. The disk appears relatively thin and elongated with a reddish hue to it. Within the disk, a slight warping is suggested. No distinct spiral arm structures can be discerned at this viewing angle. There is no evidence of significant tidal disturbances or ongoing mergers. This appears to be a quiescent system, though with hints of star formation. 
