The galaxy presents as a merging system, with two distinct nuclei visible. The primary nucleus appears more concentrated and has a yellowish hue, suggesting an older stellar population. The secondary nucleus is less defined, appears more diffuse, and has a more orange-red color, potentially indicating ongoing or recent star formation. There is evidence of tidal distortions or extended features between and around the nuclei, suggesting ongoing gravitational interaction. The overall structure is not highly organized, with an irregular shape and a relatively smooth texture, but it appears slightly elongated. The blue light is not well represented, suggesting an older stellar population is the primary constituent of the galaxy.
