The galaxy presents a largely smooth morphology. Its shape appears to be somewhere between round and elliptical, with a slight elongation visible. The central region exhibits a high degree of concentration and a yellow-red hue, indicative of an older stellar population. There is a hint of a faint, diffuse halo surrounding the central bulge. No distinct spiral arms or prominent dust lanes are discernible in this image. Any signs of mergers or major disturbances seem to be nonexistent or minimal. The color suggests that recent star formation activity is relatively low or absent. 
