This galaxy appears to be an elliptical galaxy, displaying a smooth, largely featureless morphology. It exhibits a predominantly round shape. The galaxy's color profile suggests a higher concentration of older stellar populations, giving it a reddish-yellow hue. There are no visible spiral arms or dust lanes, characteristic of spiral galaxies. The overall structure is relatively undisturbed, showing no significant signs of recent or ongoing major mergers. The galaxy appears to be a relatively isolated system within its immediate vicinity. The light appears to be concentrated in the center, indicating a possible supermassive black hole.
