The observed galaxy appears to be a disk galaxy, viewed at a near edge-on inclination. The central bulge is bright and elongated along the plane of the disk, exhibiting a roughly elliptical morphology. Some light from the disk is visible, and it appears to have a warped morphology. Faint tidal features may be present, suggestive of possible past interactions or a minor merger. There is a hint of a disk structure, but it is not well defined. The overall color is consistent with a population of relatively old stars, with some regions of possible younger, bluer stellar populations. The galaxy is surrounded by a faint halo of diffuse light. Based on its structure and possible interactions, the galaxy appears to be in a late stage of morphological evolution.
