The galaxy presents a generally smooth and rounded morphology. It appears to be relatively compact, with a concentrated central region. There is some evidence of a radial color gradient, with the central region displaying a more yellowish hue compared to the outer regions, which exhibit a slightly bluer tint. This color difference might indicate variations in stellar populations or dust content within the galaxy. There is no obvious presence of spiral arms or a bar structure. The overall appearance suggests a galaxy without major ongoing interactions or disturbances, although there is a very slight asymmetry.
