The galaxy presents a predominantly smooth, elliptical morphology. The central bulge appears bright and concentrated with a yellowish hue, suggesting an older stellar population. Fainter, more diffuse structures extend outwards, exhibiting a slightly bluer tint compared to the core, potentially indicating areas of more recent star formation. There is evidence of a possible minor disturbance or tidal feature visible as a faint extension on one side of the galaxy. The overall shape suggests a system that may be evolving towards a more relaxed state, although it is still shows some signs of dynamic activity.
