The galaxy presents a generally smooth, elliptical morphology. The core region exhibits a concentrated, bright golden hue, suggesting a population dominated by older stars. Moving outward from the center, the color gradually shifts towards a slightly redder tone, possibly indicative of an increasing fraction of older stellar populations. The galaxy appears largely undisturbed, with no obvious signs of recent merger activity or significant tidal features. There is a slight deviation from perfect circularity, leaning toward an in-between, rather than perfectly round, shape. Overall, the galaxy’s characteristics suggest a mature elliptical galaxy with a substantial stellar mass and a low rate of ongoing star formation.
