The galaxy presents a generally smooth and elliptical morphology. It appears centrally concentrated with a bright, yellowish core that gradually diffuses outwards into a less defined halo. There is a subtle elongation to the galaxy's shape, suggesting it is not perfectly spherical but rather somewhat flattened. Evidence of any spiral arm structure or significant dust lanes is absent from the image. The galaxy's color gradient suggests older stellar populations are dominant. The overall appearance points towards an early-type galaxy, likely an elliptical or lenticular type. No significant tidal features or indications of recent major mergers are discernible. Faint, subtle disturbances are possible within the extended halo region, but further investigation is needed to confirm their nature.
