The galaxy presents a generally smooth morphology with a slight elongation, suggesting an elliptical or lenticular classification. The light distribution indicates a high degree of central concentration, with a bright, well-defined nucleus. The galaxy exhibits a color gradient, with the core appearing more yellow-orange and the outer regions transitioning to a slightly bluer hue. There is no visible spiral arm structure or dust lanes. Minimal signs of tidal disturbances or active galactic nuclei are present, though a subtle asymmetry hints at a possible past interaction or minor merger event. The overall appearance suggests a mature stellar population with a relatively low ongoing star formation rate.
