The galaxy presents a largely smooth morphology, exhibiting a centrally concentrated luminosity profile. It appears approximately elliptical in shape, with a high degree of roundness. Evidence of a disk-like structure is minimal. The galaxy's color suggests a moderate level of star formation activity, potentially higher in its central region based on the apparent color gradients. There are no immediately obvious signs of major mergers or significant tidal disturbances in the image. Subtle color variations might indicate localized regions of star formation or dust obscuration.
