The galaxy presents a predominantly smooth morphology. The central region exhibits a concentrated, bright core, suggesting a high stellar density. The overall shape appears largely spheroidal, deviating slightly from a perfect circle. Faint, diffuse extensions are potentially visible surrounding the main body, though their nature is uncertain. A faint galaxy is visible, positioned close to the primary galaxy. There is no strong evidence of significant tidal disturbances or ongoing major merger events. Minor irregularities or subtle features in the galaxy's structure cannot be fully excluded based on this image alone. Further analysis across multiple wavelengths is required to assess the nature of these features.
