The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge that dominates the overall light profile. The galaxy appears to be relatively undisturbed, showing no prominent tidal features or signs of a major merger event. The color is generally consistent across the galaxy. There may be a very slight disk structure, but it is not clearly defined. The smooth appearance suggests that star formation is not currently a dominant process within the galaxy. The majority of the light emitted appears to be from older stellar populations, with minimal presence of younger, bluer stars. It presents with a round overall structure. 
