The galaxy presents as a somewhat diffuse object. It exhibits an irregular morphology, showing hints of disk-like structure, but with significant disturbances. The central region is brighter and more concentrated, suggesting a central bulge or nucleus.

Color gradients are visible within the galaxy. The central regions exhibit a slightly redder hue, potentially indicating an older stellar population. The outer regions, while faint, appear bluer, possibly indicative of ongoing star formation. The overall faintness and irregular features suggest a lower mass system with modest star formation activity. Evident distortions in the main galactic body imply possible interactions or merger events in the galaxy's recent past. There may be signs of tidal debris or disrupted structures further supporting merger activity.
