The galaxy presents as a roughly elliptical structure, viewed at an angle between face-on and edge-on. A prominent central bulge is observed, exhibiting a yellowish-white hue, suggesting an older stellar population. Surrounding the bulge is a disk component that displays a bluer color gradient. Faint spiral arm structures are suspected within the disk, however the image quality is not sufficient to make any conclusions. The disk extends further than the bulge, defining the overall shape of the galaxy. The smoothness of the disk suggests that the galaxy has not recently undergone a major merger event. No significant tidal features or strong disturbances are observed, but minor disturbances cannot be ruled out. There is a weak indication of a central bar structure within the galaxy. The overall morphology indicates a relatively evolved galaxy, possibly an intermediate spiral type.
