The galaxy presents as a centrally concentrated, elliptical-like system. It exhibits a smooth morphology with a dominant spheroidal component. The light profile appears relatively uniform, indicative of an older stellar population and a lack of prominent spiral arms or active star formation regions. The color is generally redder, suggesting a population of evolved stars. There is only minor evidence of possible disturbances within the galaxy's structure, such as faint tidal features or asymmetries.
