The galaxy presents as an elliptical morphology, appearing mostly smooth in texture. The overall color gradient suggests a higher concentration of older stellar populations, trending towards redder wavelengths. The object has a slight elongation along its major axis, but generally exhibits a rounded form. There is no noticeable presence of spiral arms, dust lanes, or active galactic nuclei. The morphology suggests it is likely a passively evolving system, with little evidence of ongoing star formation. There is no indication of major mergers or significant tidal disturbances.
