The galaxy presents a largely smooth and rounded morphology. Its color profile suggests a dominant population of older stars, exhibiting a yellowish-orange hue that concentrates towards the galactic center. This central region is the brightest and most densely packed portion, with intensity diminishing radially outwards. There is no apparent spiral structure, bar, or significant disk component visible in this image, which suggests a more spheroidal shape. Minor asymmetries or disturbances may exist, but the overall impression is of a fairly relaxed system, implying a low rate of ongoing star formation. The galaxy appears relatively isolated, with no obvious signs of recent or ongoing merger activity.
