The galaxy appears as a centrally concentrated elliptical with an overall smooth morphology. The light profile is relatively well-defined, with a core that exhibits the highest surface brightness, gradually decreasing outwards. There is a slight elongation, indicating it is not perfectly spherical, and the main body of the galaxy shows some evidence of underlying disk features, although they are not prominent, with a tilt of about 30 degrees. The color is predominantly bluish-white, suggesting a moderate population of younger, hotter stars, but is not a very active star forming area. There is a small disturbance in the lower corner, suggesting possible tidal disruptions or mergers.
