The galaxy appears as a somewhat smooth, elliptical-like object. It exhibits a centrally concentrated luminosity profile, with a bright core that diminishes gradually towards the outer regions. There is a slight hint of a disk-like structure, but this is not clearly defined. The galaxy's color is primarily yellowish-white, with hints of redder hues, particularly towards one side, possibly indicating regions of ongoing or recent star formation. The overall appearance suggests that the galaxy is relatively evolved and likely contains a significant population of older stars. There are some irregularities observed in the morphology, indicating some possible ongoing or past merger events. The galaxy is generally round in shape, and its apparent lack of strong spiral arms or a bar structure supports the classification of either an elliptical or lenticular galaxy.
