The galaxy presents as a singular object with a high degree of central concentration, exhibiting a largely smooth morphology. It appears somewhat round. The galaxy does show hints of minor disturbances in its overall structure, possibly suggesting minor tidal interactions or internal asymmetries. There's a slight deviation from perfect symmetry, with a subtle elongation that could indicate a weak bar structure or a past merger event. Based on the color profile, it shows light emission in green and blue, indicative of younger, hotter stars and active star formation regions. Overall, the galaxy presents a blend of smooth, evolved features with subtle hints of dynamic activity.
