The galaxy presents a generally smooth morphology, with a high degree of central concentration. The light is more concentrated in the center and gradually decreasing towards the edges. This is indicative of a relatively relaxed system. The galaxy exhibits a slight elongation, though it is largely spheroidal in appearance. Subtle color gradients are present, with the core exhibiting a warmer, possibly redder hue, transitioning to cooler, bluer tones in the outer regions. There may be some minor disturbances in the outer regions of the galaxy, but the overall structure indicates a well-defined system without any obvious signs of a recent major merger event. The size appears to be of average size for a galaxy at its distance, without any extreme features or grand design structures. The low star formation rate supports the smoother overall morphology.
