The galaxy presents a relatively smooth morphology, appearing largely elliptical or spheroidal. The light distribution is centrally concentrated with a gradual falloff in surface brightness moving outward from the core. There is a slight elongation, but overall the shape is close to circular. The galaxy exhibits a color gradient, with the central region appearing slightly redder, likely indicating an older stellar population. The outer regions show a hint of bluer color, possibly suggesting the presence of younger stars. The galaxy appears to be relatively isolated, showing no prominent signs of tidal interactions or major disturbances in its morphology. There is a very faint suggestion of a diffuse halo surrounding the main body of the galaxy.
