The galaxy presents as a centrally concentrated, elliptical-like structure. It exhibits a smooth, mostly featureless morphology, with a high degree of central light concentration that appears nearly spheroidal in shape. There's no immediately obvious evidence of spiral arms or a distinct disk component. The light distribution suggests a primarily older stellar population, with color information indicating a redder overall hue, indicative of evolved stars. There are no clear indications of any ongoing major merging events or significant tidal disturbances.
