The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge that is yellowish in color. This suggests an older stellar population dominating the core region. The outer regions show a gradual decrease in luminosity and a subtle color shift towards slightly bluer hues, potentially indicating the presence of younger stars within the extended galactic halo. No obvious spiral arm structures or prominent dust lanes are discernible, reinforcing the classification of a galaxy with primarily evolved stellar populations. There are hints of some very faint, small disturbances outside of the main body of the galaxy. The galaxy's round shape also supports this idea.
