The galaxy presents a largely smooth, elliptical morphology. Its overall shape appears round, lacking any significant elongation or asymmetry. There is a central bulge, visually dominant and exhibiting a reddish-orange hue, indicative of an older stellar population. The outer regions of the galaxy, while still smooth in appearance, transition to a bluer color, suggestive of the presence of younger, hotter stars in these areas. There is no apparent spiral structure or prominent disk visible. No tidal tails or other signs of recent major merger events are evident, although subtle irregularities in the outer regions could indicate minor interactions.
