The galaxy presents as a roughly elliptical system with a notable bulge component. The light distribution appears centrally concentrated, exhibiting a smooth gradient with a high degree of symmetry. The isophotes are elongated, possessing a ratio of the semi-minor to semi-major axis of approximately 0.7. There's evidence of faint, diffuse extended emission surrounding the galaxy. The core of the galaxy displays a yellowish hue, which gradually transitions to a bluer color in the outer regions. There may be a subtle disk component to the galaxy, but that is difficult to tell.
