The observed galaxy presents an elliptical morphology, exhibiting a smooth light distribution. The galaxy core shows a concentrated region of yellow-white emission, potentially indicating an older stellar population. The extended regions display a reddish hue, possibly suggesting ongoing or recent star formation. There is a slight hint of a blue region adjacent to the central bulge on one side, which may show younger star formation in one part of the galaxy. There appears to be a very slight degree of disturbance. The object is relatively isolated. Its overall structure suggests a gravitationally bound system undergoing evolution.
