The galaxy presents as a moderately luminous, relatively smooth object with an elliptical morphology. The central region exhibits a high degree of concentration, characterized by a yellowish-white hue suggesting an older stellar population. Moving outward from the core, the light gradually decreases. There's a subtle transition to a more bluish tinge in the outer regions, possibly indicating the presence of younger, hotter stars, or a different dust composition. The overall shape leans towards being elongated, but the round fraction is high, with no apparent spiral arms or distinct features. The galaxy appears isolated, showing no visible signs of tidal interactions or major disturbances. The morphology suggests it is not undergoing a major merger and presents minimal signs of on-going star formation.
