The galaxy appears to be a spiral galaxy, viewed nearly edge-on. A dust lane is obscuring part of the central bulge, and is also evident in parts of the disk. The disk appears asymmetric, with one side potentially slightly more extended than the other. The central bulge is prominent and exhibits a smooth, yellowish color, suggesting a population of older stars. The disk shows hints of bluer regions, consistent with younger stellar populations, but these regions are not well-defined, which hints at low star formation rates. There is no visual indication of a major ongoing merger or significant tidal disturbance. The overall shape seems fairly regular and undisturbed.
