The galaxy appears as a centrally concentrated object, exhibiting a smooth, elliptical morphology. The core region displays a bright, yellowish-white luminosity, suggesting a significant population of older stars. There is a subtle transition to a bluer hue surrounding the central region, potentially indicating the presence of younger stellar populations and some ongoing star formation. The galaxy appears relatively isolated with no obvious signs of tidal interactions or major disturbances, with a smooth overall structure and shape.
