The galaxy presents as a flattened, disk-shaped structure viewed edge-on. A prominent central bulge is visible, appearing smooth and concentrated with a yellow-orange hue, suggesting an older stellar population. The disk component appears relatively thin and extends outwards from the bulge, exhibiting a bluer color gradient. There is no apparent evidence of significant dust lanes or spiral arm structures. The galaxy has a relatively low star formation rate. It shows a large, fairly substantial mass. There are no visible signs of tidal disturbances or ongoing mergers. The bulge shape is rounded. The colors appear to be mainly yellow and red, with little blueness on the disk.
