The galaxy presents as a somewhat diffuse object, with a moderate degree of internal structure. The overall shape appears irregular, possibly exhibiting signs of tidal disturbances or ongoing interactions. A dominant central bulge is not readily apparent.

The light distribution is uneven, suggesting a patchy mix of stellar populations. Blue-ish hues are observed, potentially indicative of recent star formation activity. Areas showing a more red-shifted light are also seen, likely corresponding to older stellar populations. There is no clear spiral arm structure visible. The galaxy has a flocculent texture, appearing to have a clumpy morphology. It appears to be in some state of interaction.
