The galaxy presents as an elliptical morphology, exhibiting a smooth, diffuse light distribution. A central bulge region appears bright and concentrated, with a color gradient shifting toward redder hues. The outer regions of the galaxy fade gradually, displaying a bluer tint relative to the core, hinting at the presence of some younger stellar populations within the disk. There is a slight asymmetry or minor disturbance in the galaxy's shape, potentially indicating an ongoing or recent interaction. Although there is some subtle structure visible, the overall appearance suggests a system with well-mixed stellar populations.
