The galaxy appears to be a relatively smooth, centrally concentrated system, likely an elliptical or lenticular galaxy. It exhibits a bright, compact core, gradually fading into a more diffuse halo. The overall shape is approximately round. There is a hint of a faint, slightly extended disk-like structure around the central bulge, though it is not sharply defined. No prominent spiral arms or significant dust lanes are discernible. The color profile suggests a generally older stellar population, with a reddish hue concentrated in the core and a slightly bluer tint in the outer regions, potentially indicating some ongoing, albeit low-level, star formation. There are no obvious signs of any major ongoing merger events or tidal disturbances. The general appearance indicates a galaxy that is relatively evolved and dynamically stable.
