The galaxy presents as a relatively smooth, elliptical structure. It appears to be lenticular in shape. The central region exhibits a high surface brightness, indicative of a concentrated stellar population or active galactic nucleus. Moving outwards from the core, the brightness decreases gradually, and appears to fade out smoothly. The outer regions of the galaxy display a diffuse glow. There may be some dust lanes present, but are difficult to distinguish. No significant tidal features or signs of major merger activity are immediately apparent.
