The observed galaxy presents a predominantly smooth morphology, exhibiting a largely featureless structure. Its shape is broadly elliptical, appearing nearly round in projection. There is a suggestion of a possible minor disturbance in its morphology, but overall the system appears relatively undisturbed. The galaxy exhibits a distinct color gradient, transitioning from bluer hues in its central regions to redder colors in its outer peripheries. This suggests a radial variation in stellar populations, with a centrally concentrated population of younger, hotter stars, and older, cooler stars dominating the outer halo.
