This galaxy presents as a relatively smooth, elliptical structure. There is a central, highly luminous bulge that dominates the galaxy's overall appearance. The light is concentrated and bright, appearing slightly yellowish-white at the core, suggesting an older stellar population and/or dust obscuration. 

There is evidence of possible tidal interactions or an ongoing merger event. A smaller, more diffuse companion object is visible in close proximity to the main galaxy. There appears to be a slight visual disturbance or plume extending away from the brighter galaxy, possibly indicating gravitational interaction. 

The galaxy's red shift suggests it is a relatively distant object. The size and luminosity indicate that it is a fairly massive galaxy, despite its distance.
