The galaxy presents as an elliptical morphology, characterized by a smooth and concentrated light distribution. The overall shape appears nearly circular, with a high degree of central concentration. There is no apparent disk structure or spiral arm features visible. The galaxy exhibits a color gradient, transitioning from a relatively brighter, yellowish core to fainter, slightly redder outer regions. There is no apparent evidence of tidal tails, strong asymmetry, or other obvious signs of recent or ongoing major merger activity. Minor disturbances may be present but are not readily discernable. The galaxy’s color and morphology suggest an evolved stellar population and relatively low current star formation activity.
