The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a generally elliptical morphology, appearing mostly round with minimal elongation. There is faint evidence of some features or disturbances. It is a galaxy that is not currently undergoing any major mergers, although there is a hint of minor disturbances or possible past interactions. The galaxy's overall color suggests a population dominated by older stars, potentially with limited ongoing star formation. It possesses a considerable mass.
