The galaxy presents as a disk galaxy, oriented almost perfectly edge-on from our vantage point. A prominent central bulge is visible, exhibiting a smooth, rounded morphology. The disk component appears relatively thin and elongated, with a discernible dust lane bisecting the galaxy along its major axis, obscuring light from the far side of the disk. There are hints of possible minor tidal disturbances or interactions in the outer regions of the disk. The overall colour gradient suggests a relatively old stellar population, as the light is redshifted and therefore appears redder.
