The galaxy presents an elliptical morphology, exhibiting a smooth and concentrated light distribution. The central region displays a yellow-orange hue, likely indicative of an older stellar population. There appears to be a subtle transition towards a faint, greenish-blue outer envelope. The galaxy does not show prominent spiral arms or any clear signs of active star formation. There are suggestions of minor asymmetry that may be tidal in nature. The galaxy appears largely undisturbed, with no immediately obvious signs of ongoing or recent major merger activity.
