The galaxy appears to be a luminous, elliptical galaxy with a smooth morphology. It presents as a concentrated, roughly circular object with a bright central core that gradually fades toward its outer regions. The color profile suggests a population of older stars, as evidenced by the reddish-yellow hue. There are no clearly defined spiral arms or dust lanes visible, indicating a lack of significant ongoing star formation. The overall structure suggests a galaxy that has largely completed its merger history, exhibiting minimal signs of tidal disturbances or interactions. The galaxy seems to be well-evolved, with a relatively homogeneous stellar population.
