The galaxy presents as a relatively smooth, elliptical morphology, elongated along its major axis. It exhibits a concentrated central bulge, appearing a yellowish-orange hue, indicative of an older stellar population. The outer regions of the galaxy show a slight bluer tint compared to the core, suggesting the presence of a younger stellar population though the overall color is still on the redder side. The galaxy appears relatively isolated. There is a low probability of a merger event affecting the galaxy. The overall structure suggests a galaxy that has largely ceased significant star formation activity, and the mass is expected to be large. 
