The object appears to be a relatively smooth galaxy with a concentrated central bulge. There is a slight elongation of the galaxy suggesting it may not be perfectly spherical. The color is predominantly yellow, indicative of an older stellar population with fewer young, massive stars. There is no obvious spiral structure or dust lanes visible. There is a very slight asymmetry on the outskirts of the galaxy, which could be indicative of a minor disturbance to the galaxy. The galaxy appears to be isolated, showing no signs of a major merger. 
