The galaxy presents a largely smooth morphology, with minimal discernible features such as spiral arms or a prominent disk structure. The light distribution suggests an elliptical shape, tending towards a less-rounded, slightly elongated form. Color gradients are subtle, with a hint of a yellowish-orange hue concentrated in the central region, possibly indicating an older stellar population. The outer regions appear bluer, potentially signaling the presence of younger stars or ongoing, albeit limited, star formation. There is no apparent major disturbance or merging activity visible in the immediate vicinity of the galaxy. The galaxy's overall appearance points towards a system that is relatively evolved and dynamically settled, rather than undergoing significant interactions or rapid starburst events.
