This galaxy appears to be a relatively smooth, elliptical or lenticular galaxy. The light distribution exhibits a centrally concentrated, roughly ellipsoidal morphology. The overall color suggests a moderate presence of older stellar populations, with a slightly redder hue in the central regions, indicating potentially higher metallicity.

There is a subtle hint of possible tidal interaction or minor disturbance, manifested as a slight asymmetry or extension in one direction. This could possibly be caused by a small merger, however there is nothing significant in the image to indicate the presence of tidal tails. 
