The galaxy presents a somewhat smooth morphology, though with discernible features. It appears generally rounded in shape. There may be a minor disturbance occurring or a potential merger event in progress, as the galaxy appears to have multiple nuclei or a disturbed central region. Color gradients suggest the presence of varying stellar populations and ongoing star formation. The galaxy exhibits a substantial amount of light output, especially in the redder wavelengths, potentially indicating an older stellar population mixed with younger, actively forming stars. The overall impression is that of a galaxy in a dynamic state, possibly undergoing interactions that influence its structure and stellar formation.
