The galaxy presents as a relatively smooth, elliptical structure. The central region exhibits a high degree of luminosity, appearing intensely yellow-white, suggesting a concentration of older stellar populations. A slight elongation is observed, though the galaxy does not deviate substantially from a rounded form. There is little evidence of prominent spiral arms or distinct features such as dust lanes. The overall impression is of a mature galaxy with a high degree of sphericity and little ongoing star formation. Minor asymmetry hints at a past or ongoing interaction, however, overall the galaxy's structure appears relaxed and undisturbed. The outer regions fade gradually into the background, suggesting a smooth density profile. 
