The galaxy presents a predominantly smooth morphology, with a noticeable lack of defined spiral arms or a prominent disk structure. Its shape is roughly intermediate between round and elliptical, displaying a slight elongation. The galaxy exhibits a color gradient, appearing brighter and more yellow-red towards the center, suggesting a higher concentration of older stellar populations in the core. The outer regions of the galaxy appear fainter and slightly bluer, potentially indicating the presence of younger stars or a lower density of stars. There is no obvious evidence of a major ongoing merger event, although there might be a minor irregularity or disturbance in the galaxy's shape, hinting at a possible past interaction. The overall appearance suggests a relatively evolved galaxy with a quiescent star formation rate.
