The galaxy presents a largely smooth, elliptical morphology, appearing as a diffuse, centrally concentrated light source. The core region exhibits a yellowish-white hue, suggesting a population of older, cooler stars. Moving outwards from the core, a subtle gradient towards a bluer colouration is observed, potentially indicating the presence of some younger stellar populations in the galaxy's outer regions. Overall, the galaxy shows no obvious signs of strong spiral structure or major disturbances, but there are hints of a minor irregularity along its edges, perhaps resulting from a past interaction. The galaxy appears relatively isolated, based on the immediate field.
