The galaxy presents as a predominantly smooth, elliptical structure with a high degree of central concentration. It exhibits a generally featureless morphology with a near-circular isophotal shape. There is minimal evidence of spiral arm structure or dust lanes. The color gradient is relatively smooth, with a bluer hue in the outer regions gradually transitioning to a redder, yellower core, suggesting an older stellar population concentrated towards the center. There might be some minor distortions or asymmetries visible, possibly indicative of a previous or ongoing minor interaction, although a clear merger event is not immediately apparent. The light distribution suggests a relatively old and evolved system with a low rate of current star formation.
