The galaxy presents as a diffuse, moderately luminous object. The overall morphology appears relatively smooth, although subtle features are present. There's a slight central condensation of light, indicating the presence of a bulge or a higher concentration of stars in the nuclear region. 

A faint, extended disk-like structure surrounds the central bulge. The galaxy's color is predominantly bluish, suggesting ongoing or recent star formation activity. There are hints of slightly redder regions within the disk, potentially indicating areas with older stellar populations or dust obscuration. The galaxy does not show any obvious signs of a major ongoing merger, although there may be minor disturbances in its morphology suggesting past interactions or internal dynamics affecting its structure.
