The galaxy presents as a disk-shaped object, viewed nearly edge-on from our vantage point. A prominent central bulge is evident, displaying a concentrated luminosity. The bulge appears to be roughly spherical and yellow/orange in color.

The disk component is considerably fainter and bluer than the bulge. The apparent dust lane is subtle but seems to be present within the disk, bisecting the central bulge, implying a significant obscuration. No distinct spiral arm structures are discernible in the disk, this may be due to the limitations of the resolution or the viewing angle.

There appears to be a slight warp or asymmetry to the disk, with one side seeming slightly more extended than the other. No tidal tails or obvious signs of a major merger event are apparent, although the faintness of the disk and the viewing angle make it difficult to rule out minor interactions.
