The galaxy presents a generally smooth, elliptical morphology. It is centrally concentrated with a bright core that gradually fades into a more diffuse halo. The light distribution is relatively uniform, lacking any prominent spiral arms or significant substructure. There is a slight elongation to its shape, suggesting it's more lenticular than perfectly spherical. The galaxy's color profile indicates an older stellar population, appearing redder overall with a subtle blue component in the outer regions. There is no strong evidence of ongoing mergers or tidal disturbances, and the structure seems well-settled.
