The galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a bright, concentrated bulge with a yellowish hue, suggesting an older stellar population and reduced star formation activity within the core. Moving outward from the center, the light gradually fades into a more diffuse halo. The overall color gradient indicates a possible transition in stellar populations, with potentially younger, bluer stars contributing to the outer regions. There may be some minor asymmetry to the overall distribution of light, but no obvious signs of significant disturbance or interaction with other galaxies.
