The galaxy presents as an edge-on spiral or lenticular type, exhibiting a prominent central bulge that is significantly brighter than the surrounding disk. The bulge appears smooth and elliptical in shape, with a major axis aligned vertically in the image. The disk is relatively thin and elongated, appearing to extend outwards from the bulge in both directions.

There is a noticeable dust lane or obscuration running along the mid-plane of the galaxy, bisecting the bulge and disk. This feature gives the galaxy a less smooth appearance in the optical wavelengths. The outer regions of the disk fade gradually, and it shows some irregularities in its shape with the disk being more extended on one side. There is no obvious spiral arm structure visible at this resolution, possibly due to the edge-on orientation. Overall, the galaxy exhibits an elliptical light distribution, with the intensity decreasing from the central bulge outwards.
