The galaxy presents as a relatively smooth, elliptical structure with a high degree of central concentration. Its morphology is predominantly spheroidal, lacking any readily discernible spiral arms or a prominent disk component. The color profile indicates an older stellar population, showing a redder hue towards the central region, consistent with a lack of ongoing star formation. There is a slight elongation of the galaxy's shape, with a moderate ellipticity, but no signs of any major merger events or significant tidal disturbances. Overall, the galaxy exhibits characteristics consistent with a passively evolving elliptical galaxy at intermediate redshift.
