The galaxy presents an overall smooth appearance, with a somewhat elongated, elliptical shape. It exhibits a distinct color gradient, transitioning from a yellowish-white core to a bluer outer region. The central region is the brightest, suggesting a high concentration of older stars, while the outer region hints at the presence of younger stellar populations and possible ongoing star formation. There is no obvious spiral structure or prominent dust lanes visible; the morphology appears relatively featureless, without signs of major disturbances or merging activity.
