The galaxy presents as a spiral, observed from an edge-on perspective. A distinct dust lane is not readily apparent in the image, however the galaxy exhibits a clear central bulge. The bulge appears relatively smooth and elongated. The galactic disk shows some clumpy features suggestive of stellar formation regions or irregular dust distribution. The galaxy does not show strong signs of major ongoing merger activity, though a degree of minor disturbance may be present as seen by the asymmetric glow of the top disk in the image. The color of the galaxy appears more blue, which could indicate active star formation.
