This galaxy presents as a disk galaxy, observed nearly edge-on. A prominent central bulge dominates the visual appearance with an enhanced brightness and a smooth texture. The bulge appears to be elongated with a boxy shape. A faint disk extends from the central bulge, appearing thin and relatively featureless in the image. There may be some evidence of minor gravitational disturbance, with possible asymmetries in the disk's outer regions. Overall, the galaxy seems to be relatively isolated, without obvious signs of a major merger event. The disk appears to be made of older, redder stars. 
