The galaxy appears to be a relatively smooth, elliptical system. It has a concentrated, bright core that fades gradually into the outer regions. The central region exhibits a yellowish-white hue, which might indicate an older stellar population dominating this area. Moving outwards, there are subtle color variations, transitioning to a bluer tint. This could imply the presence of younger, hotter stars in the outer regions, although the smoothness suggests any ongoing star formation is minimal. The galaxy shows a generally rounded shape with some apparent elongation. No clear spiral arms or distinct features like dust lanes are discernible. The overall structure suggests a well-evolved galaxy, potentially residing in a relatively quiescent environment. There is a very slight suggestion of a faint halo surrounding the central bulge, but further analysis would be required to confirm its presence and properties. There appears to be no interaction with any other galaxies.
