The galaxy exhibits a pronounced elliptical morphology. It appears elongated, with a high aspect ratio, suggesting a cigar-like shape. The central region displays a high surface brightness and a distinct yellowish-orange hue, potentially indicating an older stellar population and minimal ongoing star formation in the core. Moving outward from the center, the color shifts towards a slightly bluer, though still muted, tone. This could imply the presence of younger stars in the outer regions, albeit at a lower rate of formation compared to bluer, spiral galaxies. There are no discernible spiral arm structures or prominent dust lanes visible in this image. No significant signs of any ongoing merger events or tidal disturbances are apparent. The galaxy appears relatively isolated and undisturbed, suggesting it is not currently interacting strongly with other galaxies. The overall structure presents a smooth appearance, hinting at a more evolved system.
