The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits an elliptical or spheroidal morphology, lacking any apparent spiral arm structures or a well-defined disk. The light distribution appears quite uniform, with a gradual decline in intensity from the core outwards.

There are two regions of increased illumination, one brighter than the other. Both appear smooth. There are no signs of tidal tails, strong dust lanes, or other indications of recent major merger events. The color gradient is subtle.
