The galaxy presents as a single, centrally concentrated light source. Its morphology appears smooth and elliptical, lacking any prominent spiral arms or other distinct features. The color profile indicates a yellowish-orange hue, suggesting a stellar population dominated by older, redder stars. The absence of significant blue light implies a low rate of ongoing star formation within the galaxy. There is no obvious indication of a recent major merger event or significant tidal disturbances. The galaxy exhibits a high degree of roundness. Faint, diffuse extensions of light are visible in the surrounding halo, although they are not well-defined. Overall, the galaxy appears to be a relatively quiescent, massive elliptical galaxy at a moderate redshift.
