The galaxy appears to be a relatively smooth, elliptical galaxy. Its shape is nearly circular. There is a concentration of light in the center, suggesting a bulge component. There is a lack of obvious spiral arm structure. The color is a yellowish-orange hue, which may indicate an older stellar population with lower rates of current star formation. There is some indication of possible minor disturbances or tidal features, but these are difficult to discern definitively given the resolution. The galaxy's profile seems to gradually fade away from the center. There is very little evidence of dust lanes or patchy regions of star formation.
