The galaxy presents a largely smooth and elliptical morphology. The light is concentrated towards the center, forming a bright nucleus. There is a noticeable color gradient, with the core appearing yellow-white, suggesting a population of older stars, while the outer regions exhibit a slightly redder hue, potentially indicating the presence of some dust or a somewhat younger stellar population compared to the very center. The galaxy is mostly round, with no obvious signs of strong tidal interactions or major disturbances. Faint wisps extend slightly from the main body. The overall structure appears relatively undisturbed, characteristic of a galaxy that has undergone significant morphological evolution, resulting in a quiescent state. There is a subtle asymmetry in the overall light distribution, suggesting the possibility of a minor interaction or past merger event.
