The galaxy presents a generally smooth and rounded morphology. It appears elliptical in shape, with a high degree of central concentration. The light profile suggests a bulge-dominated system, exhibiting a gradual decrease in brightness from the core outwards. A slight color gradient is observed, transitioning from a warmer, possibly older stellar population in the central regions to slightly cooler tones in the outer halo. There is no obvious indication of spiral arms or a prominent disk structure. The galaxy does not show strong signs of tidal disturbances or ongoing major mergers, although minor asymmetries cannot be ruled out due to the resolution. Overall, this galaxy is characterized by a relatively evolved stellar population and a quiescent morphology.
