The galaxy appears to be a relatively smooth object with a centrally concentrated bulge. The galaxy has a noticeable but subtle disk that is oriented at a near face-on angle relative to our line of sight. There are minimal signs of distinct spiral arm structures within the disk. There is some slight blue coloration visible in the outer regions of the disk, which might indicate more recent star formation activity in those areas. The central bulge is generally white. The overall shape is close to a rounded ellipse. There is no obvious evidence of a major merger event currently in progress, although there may be some slight disturbances or asymmetries in the outer regions.
