The galaxy appears to be a spiral galaxy, seen at an oblique angle. It exhibits a bright, concentrated central bulge that graduates into a fainter, more diffuse disk. The disk shows hints of spiral arm structure, though they are not sharply defined. The overall color of the central bulge is yellowish-white, suggesting an older stellar population. The disk appears bluer, potentially indicating the presence of younger, hotter stars and ongoing star formation. The morphology is predominately smooth. There appears to be no presence of any major merging or tidal disturbances in the galaxy's morphology. The shape of the galaxy is relatively oval.
