The galaxy appears to be a relatively smooth, elongated structure, suggestive of an elliptical morphology, however, a disk component cannot be ruled out. The object exhibits a noticeable color gradient, transitioning from a more yellowish-white core to fainter, bluer outer regions. The central region appears more concentrated and brighter than the extended halo. There is little indication of significant dust lanes or spiral arm structures; any visible disk does not show much recent star formation. There is no obvious indication of any major ongoing merger activity or tidal disturbances.
