The galaxy presents as a centrally concentrated object with a relatively smooth light distribution, suggesting an elliptical or lenticular morphology. The galaxy exhibits a radial color gradient, appearing bluer in its central regions and becoming redder towards the outer edges. There is little to no evidence of spiral arm structure or prominent dust lanes. The object appears to be relatively undisturbed, with no obvious signs of ongoing or recent major merger activity. The rounded shape further supports a classification as an elliptical or early-type lenticular galaxy. Based on its colors, shape, and lack of apparent features, this is likely a massive galaxy with an older stellar population and low star formation rate.
