The galaxy presents an overall elliptical morphology, appearing somewhat flattened. Its color profile suggests a dominant older stellar population, exhibiting a yellowish-orange hue characteristic of evolved stars. There is a slight color gradient from the core outwards, with the core being somewhat redder. No distinct spiral arm structures are discernible, and the light distribution appears relatively smooth.

The galaxy displays a faint stellar halo extending beyond the main body, though its boundary is not sharply defined. The axial ratio indicates that the galaxy is not perfectly spherical but rather has an elongated shape. The surface brightness profile decreases gradually from the center, indicative of a centrally concentrated distribution of stars.

The image suggests little evidence of ongoing star formation. Overall, the galaxy appears to be a mature elliptical galaxy, likely having undergone significant evolution and quenching of star formation.
