The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape is elliptical, exhibiting a high degree of roundness with only slight deviation from perfect circularity. The galaxy's color profile suggests a dominant population of older stars, which is consistent with the object's smooth morphology and high central concentration. The presence of some bluer light in its outer regions may indicate ongoing, but low levels of star formation. There's no apparent disturbance or tidal features to suggest recent major merger activity, implying a dynamically relaxed state. The light profile decreases gradually from the center outwards, showing no sharp edges.
