The galaxy presents as an elliptical morphology, appearing largely smooth and concentrated. The central region exhibits a bright, almost stellar-like core, suggestive of an active galactic nucleus or a dense concentration of stars. The galaxy's light profile appears to follow a relatively steep decline from the center outwards, indicating a well-defined structure with minimal signs of significant tidal disturbances or recent major mergers. Subtle color gradients are visible, with a slight shift towards redder hues in the outer regions compared to the whiter core. The overall shape is slightly elongated, deviating marginally from a perfect circle with a minor axis ratio of around 0.8. There is no prominent disk structure or spiral arm features evident in the image.
