The galaxy presents as a centrally concentrated, elliptical-like object with a smooth morphology. The core exhibits a bright, yellowish-white hue, suggesting an older stellar population. Surrounding the core, there's a more diffuse, greenish-blue halo. The color gradient suggests ongoing, though perhaps diminished, star formation activity in the outer regions. There is no visible spiral structure or obvious signs of recent major mergers. However, there are hints of minor distortions or disturbances in the halo. Overall, the galaxy appears relatively isolated, without strong tidal interactions.
