The galaxy presents as a centrally concentrated object with a smooth morphology. It is primarily spheroid in shape, with an elliptical appearance. A significant fraction of its light is concentrated in the core. There is a smooth decline in luminosity from the center outwards, but the outer regions of the galaxy are faint and appear to smoothly blend into the background sky. There is no clear evidence of spiral arm structures or a prominent disk. The galaxy exhibits a slight elongation, and there's no obvious sign of any ongoing major merging events or strong tidal disturbances. The galaxy appears to be dominated by older stellar populations.
