The galaxy presents as a somewhat smooth, elliptical morphology with a slightly elongated shape. The central region exhibits a concentrated luminosity, appearing relatively bright with an apparent yellowish hue. The outer regions of the galaxy display a gradual decrease in luminosity, extending into a fainter, less defined halo. There is faint evidence of a disk-like structure within the galaxy. No signs of major mergers or significant disturbances are readily apparent within the galaxy's structure. The galaxy's color suggests an older stellar population, possibly indicating a lower rate of recent star formation.
