The galaxy appears to be a relatively smooth, elliptical or lenticular galaxy, potentially with a disk component. The core of the galaxy presents a bright, concentrated luminosity, suggesting a significant density of stars. The overall shape is elongated, but not exceptionally so, appearing somewhere between round and cigar-shaped. There are no obvious signs of a major ongoing merger or strong tidal disturbances. Faint, diffuse extensions are present, but do not represent the classical features of a spiral structure, instead forming a smooth halo with a subtle blue hue. The color indices appear to be bluer in the outskirts and redder towards the center.
