The galaxy presents a largely smooth and rounded morphology. There is a central, concentrated brightness, suggesting a bulge component. The galaxy exhibits a general bluish hue towards its center, potentially indicating the presence of younger stellar populations. Some subtle reddish tinges appear around the edge of the galaxy, but this is less apparent. There is no clear evidence of spiral arm structures or a prominent disk; the overall form indicates an elliptical galaxy or a lenticular galaxy viewed face-on. There are no obvious signs of strong tidal interactions or major disturbances in its structure. The galaxy appears relatively isolated and exhibits a general lack of significant recent star formation based on color.
