The galaxy presents a largely smooth morphology, appearing elliptical in shape. A bright, concentrated central bulge is apparent, suggesting a significant population of older stars. The outer regions of the galaxy exhibit a faint, diffuse halo, with a gradual decrease in luminosity from the center outwards. There may be some slight indication of a disk, but the overall structure is dominated by the central bulge, which accounts for the majority of the galaxy's luminosity. There is no strong evidence of recent merger activity or major disturbances affecting the overall structure of the galaxy. The color profile suggests an older stellar population, based on its redder color. There may be some hints of bluer regions, which would imply recent star formation. The galaxy is neither particularly round nor extremely elongated, presenting as somewhat in between.
