This galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a high degree of concentration, appearing as a bright, nearly spherical bulge with a yellowish hue, suggesting an older stellar population. There is a gradual decrease in luminosity moving outwards from the core. No distinct spiral arms or prominent dust lanes are visible, indicating that the galaxy is unlikely to be a spiral galaxy. The slight deviation from perfect sphericity suggests a possible degree of rotational support or perhaps a past or ongoing interaction with another galaxy, although no tidal tails or obvious signs of a major merger are evident in this image. The faint blueish color in the outer regions hints at some ongoing star formation, although at a low rate relative to its overall mass.
