The galaxy appears as a single, relatively smooth, and concentrated object with a reddish-orange hue. There are hints of slight disturbances in the morphology with an asymmetrical light distribution, which could indicate minor tidal interactions or internal instabilities. It is generally elliptical in shape, displaying a high degree of central concentration, suggesting an older stellar population. The object exhibits a color profile consistent with evolved stars and potentially a moderate amount of dust obscuration. Star formation activity appears to be low. Overall, the galaxy presents as a morphologically evolved system, likely a massive elliptical galaxy at moderate redshift.
