The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. The light distribution suggests a higher density of stars towards the galactic center, gradually decreasing outwards. The central region exhibits a bright, somewhat bluish-white hue, indicating a population of relatively young, hot stars or active galactic nucleus activity. The outer regions of the galaxy are fainter and show a subtle shift towards redder colors, implying a population of older, cooler stars. While there may be some underlying structure, such as a disk or spiral arms, the galaxy's features are subtle and the galaxy is dominated by its smooth, elliptical form. There is no obvious sign of recent or ongoing merger activity that visibly disrupts the overall structure. The galaxy has an intermediate roundness.
