The galaxy presents a largely smooth and rounded morphology. The color profile suggests a centrally concentrated population of older stars, exhibiting a reddish-orange hue that fades towards the edges. There is a hint of a greenish glow around the central region, potentially indicating some ongoing, though relatively low, levels of star formation. No distinct spiral arms or a well-defined disk structure are discernible. There is no evidence of major mergers or significant tidal disturbances, supporting its generally undisturbed and evolved appearance.
