The galaxy presents an overall elliptical morphology, elongated along a major axis. The light distribution appears relatively smooth, lacking prominent spiral arm structures or distinct features. There is a noticeable color gradient, transitioning from a yellowish-orange central region to a bluer periphery. This might be due to a concentration of older stellar populations towards the core and younger stars in the outer regions, indicative of potential differences in stellar formation history. While the light is generally smooth, there are hints of some disturbances or asymmetry in its shape. These might represent minor tidal interactions or internal processes disrupting the smooth profile. The galaxy appears to have a high mass and low star formation, as can be observed in the redder core and bluer outer regions, suggesting an older galaxy. There is a faint, diffuse halo surrounding the main body of the galaxy.
