The galaxy presents an overall elliptical morphology. It exhibits a smooth, largely featureless structure, with a gradual increase in luminosity towards the central region. The core appears bright and concentrated, suggesting a substantial stellar population. There's a noticeable color gradient, transitioning from a yellowish-white core to a redder, more diffuse outer halo. No distinct spiral arms or prominent dust lanes are visible. There is a subtle asymmetry in the outer regions, possibly indicating a minor gravitational disturbance or interaction. The general appearance suggests a relatively evolved system with a moderate rate of star formation.
