The galaxy presents a morphology that is difficult to classify definitively due to apparent image artifacts. However, some structural features are observable. 

The object exhibits a diffuse, extended halo. Within this halo is a core region that is brighter and more concentrated. This core region may have some faint wispy arms. There also appears to be a dust lane or some kind of obscuring band that traverses across the galaxy, possibly bisecting the core.

There may be some minor disturbance in this system, as evidenced by the asymmetry and potential tidal tails or debris surrounding the main body.
