The galaxy presents as a centrally concentrated object, exhibiting a relatively smooth and featureless morphology. There is a bright, well-defined core, suggesting a significant concentration of stellar density or an active galactic nucleus, though the resolution limits further characterization of the core. The galaxy's overall shape is generally elliptical, appearing almost round, with a gradual decrease in luminosity extending outwards from the central region. There is some subtle color variation, with a yellowish-white hue in the core transitioning to a more bluish-white outer region, suggesting a difference in stellar populations and/or star formation activity. The absence of prominent spiral arms or dust lanes indicates that this is likely an early-type galaxy. There is no obvious evidence of tidal disturbances or ongoing mergers, although faint asymmetric features cannot be ruled out at this resolution.
