The galaxy presents as a generally smooth, elliptical-like structure. The central region exhibits a high degree of concentration with a bright, yellowish-white core, suggesting a dense population of older stars. Moving outwards from the center, the light gradually fades. The elongated shape suggests the galaxy is viewed at an angle. There is a faint blueish hue at the bottom of the image, indicating possible ongoing star formation. Overall, the galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions. The color gradient from the core outward suggests a potential age gradient in the stellar populations, where the core consists of older stars and the outer regions may contain younger stellar populations.
