The galaxy presents a generally elliptical morphology. The central bulge exhibits a bright, concentrated luminosity, indicating a high density of stars. This light appears yellowish, suggesting an older stellar population. The surrounding galactic disc is less defined, showing a smoother distribution of light and a subtle bluish tint implying some ongoing, albeit possibly low, star formation. There's no clear indication of spiral arm structures, and the overall texture is relatively smooth, suggesting a lack of significant recent merger events or major disturbances. The overall roundness suggests the system is not edge-on, and could be close to face on. The galaxy shows no pronounced tidal features or dust lanes in this image.
