This galaxy appears to be a relatively smooth, elliptical galaxy. Its light profile shows a high degree of central concentration, with a bright, yellowish core gradually fading into a more diffuse, bluish halo. No distinct spiral arm structures are discernible, and the overall shape is close to circular. There is a suggestion of a slight extension, but there does not seem to be evidence of any ongoing major mergers or significant tidal disturbances affecting the galaxy's morphology. The lack of noticeable substructure or dust lanes is consistent with a more evolved stellar population. It is possible this is a galaxy that has been quiescent for an extended period. 
