This galaxy exhibits a moderately elliptical morphology, with a high degree of central concentration as indicated by the yellow-white core. Proceeding outward from the core, the galaxy shows a bluer, less concentrated disk, with a faint spiral structure perhaps present, but difficult to discern. Overall the galaxy appears to be relatively smooth, without any significant signs of ongoing or recent major mergers. There is a hint of minor disturbance present. The galaxy has a red shift placing it at a distance where its size is approximately 9 kpc in radius. Estimated to be a massive galaxy with significant star formation activity. 
