The galaxy presents a largely smooth and elliptical morphology. The central region exhibits a high concentration of light, suggesting a prominent bulge component. Progressing outwards from the core, the light gradually diminishes, indicative of a fading stellar density. There is a subtle color gradient from the core to the outer regions. The center presents a yellow-orange hue. The outer parts appear more blue. There is no clear evidence of spiral arms or a significant disk structure. Minor irregularities are present. The galaxy seems to be relatively isolated with no obvious signs of tidal interactions or major disturbances.
