The galaxy presents as a somewhat diffuse, but discernible, elongated structure. The central region displays a higher surface brightness, suggesting a condensed nucleus or bulge component. Moving outwards, the light gradually fades into a less defined disk. 

The overall color appears bluish, hinting at the presence of a younger stellar population and ongoing, but likely limited, star formation activity. There is a slight asymmetry and subtle irregularities visible, suggesting potential tidal interactions or recent minor merger activity that could be disrupting the overall galactic structure. This indicates the system could be dynamically active, but appears in a relatively evolved stage. There's an indication that part of the galaxy could be smoother than the rest.
