The galaxy presents as a relatively smooth, elliptical morphology, though not perfectly spherical. There's a noticeable concentration of light towards the center, indicating a prominent galactic nucleus. The color gradient transitions from a yellowish-white core to bluer hues in the outer regions. This potentially suggests a population of older stars concentrated in the core, with younger, bluer stars more dispersed throughout the galaxy's disk. There's a slight asymmetry in the outer regions that may indicate minor tidal disturbances or a subtle interaction with another galaxy. No spiral arm structure is visible.
