The galaxy appears as a luminous, elliptical-shaped object with a smooth, largely featureless morphology. Its color profile suggests a dominant population of older stars, with a yellowish hue concentrated towards the center and gradually fading outwards. The overall structure lacks any prominent spiral arms or dust lanes, and the absence of distinct features suggests minimal ongoing star formation activity. There is a high degree of central concentration of light. The galaxy displays no signs of recent merger activity or major disturbances.
