The galaxy presents as a relatively smooth, centrally concentrated object. Its overall morphology appears elliptical, exhibiting high degree of roundness. There is a subtle color gradient from the central region outwards, with the core appearing more yellow, suggesting an older stellar population. The outer regions are less defined, and hint at bluer colors which could suggest the presence of younger stars or ongoing, albeit possibly diminished, star formation activity. There are no prominent spiral arms or strong signs of recent major mergers, though subtle disturbances could exist in the outer regions upon closer inspection. The galaxy shows a well-defined, though not extremely compact, structure with no obvious tidal features.
