The galaxy presents as an elliptical morphology with a smooth light distribution. The core exhibits a concentrated, bright luminosity, indicating a substantial population of stars within the galactic nucleus. Moving outward from the center, the light intensity gradually decreases, suggesting a diminishing stellar density in the outer regions. There is no discernible spiral arm structure or prominent dust lanes. The galaxy's overall color appears to be slightly red-shifted. The form is generally rounded with little elongation or distortion visible in this imagery, showing no signs of major interactions or mergers.
