The galaxy exhibits a merging morphology, with two distinct components visible. One component presents a bluer color profile, potentially indicating ongoing star formation activity within this region. The second component displays a more yellow/red hue, suggesting an older stellar population or a greater presence of dust obscuring younger stars. The overall structure appears disturbed, lacking a clear, defined shape, which further supports the classification as a merging system. There is no clear central bulge. The light is somewhat diffused, with a radius of about 8 kpc.
