The galaxy presents as a moderately elliptical structure, displaying a smooth and diffuse morphology. Its color gradient transitions from a bright, yellowish core to fainter, reddish outer regions. There is no evidence of spiral arms or prominent dust lanes, suggesting it is either an elliptical or lenticular galaxy. The overall appearance indicates a system dominated by older stellar populations, with potentially limited ongoing star formation. The galaxy appears relatively undisturbed, showing no obvious signs of recent merger activity or tidal interactions. 
