The galaxy presents as a relatively smooth, elliptical-like structure. Its overall shape is notably rounded, displaying minimal elongation. The central region exhibits a significantly higher luminosity, suggesting a concentrated nucleus. The outer regions display a gradual decrease in luminosity, characteristic of a spheroid. The galaxy shows no strong evidence of spiral arm structures or prominent dust lanes. There is a possible, very minor disturbance of the galaxy, but there is little visual disturbance to the galaxy, as the luminosity and structure is very similar throughout the entire spheroid. The color profile is somewhat uniform throughout. The light emitted is on the redder side, with green being a very common color throughout the galaxy. 
