The galaxy presents a primarily smooth, elliptical morphology. It exhibits a dominant, centrally concentrated bulge, emitting strongly in the yellow-orange wavelengths. The light distribution suggests an older stellar population. The overall shape appears to be somewhat elongated, departing from a perfectly circular form. There is a subtle indication of a faint disk component surrounding the central bulge, as there seems to be slightly more defined edges in a rough plane around the galaxy. No significant spiral arm structures or major disturbances are immediately apparent. It seems to be a fairly isolated galaxy, as there are no visually obvious signs of tidal interactions or ongoing mergers. 
