The galaxy appears as a flattened, elliptical structure with a smooth light distribution. The central bulge exhibits a yellow-orange hue, suggesting a population of older stars. A disk component is subtly visible, displaying a greenish tint, which may indicate the presence of younger stars and some ongoing star formation. The galaxy's shape is elongated, leaning towards a cigar-like appearance, and shows no signs of major mergers or significant disturbances. There might be a hint of a faint spiral arm structure, but it is not strongly defined. Overall, the galaxy is likely a relatively massive system with a combination of old and intermediate-age stellar populations.
