The galaxy presents as a largely smooth, elliptical morphology. It exhibits a concentrated central bulge region with a yellowish-white color, suggesting an older stellar population. The outer regions appear somewhat less concentrated and display a slightly bluer hue. There is no obvious dust lane or spiral arm structure visible. The overall impression is of a relatively relaxed system, with no significant signs of ongoing major mergers or tidal disturbances. The light distribution appears fairly symmetrical and round. The galaxy is a significant mass and is still undergoing a moderate amount of star formation. 
