The galaxy appears to be a spiral type, though the arms are somewhat ill-defined, possibly due to its distance. The central bulge is moderately bright and appears relatively smooth in texture, showing a yellow-white color. There appears to be a slight asymmetry in the morphology, with one side of the galaxy appearing more disturbed than the other. There is evidence of some star formation within the disk, as indicated by the presence of some bluer regions, as well as redder regions that are likely older stellar populations.

There is a hint of a potential interaction with a smaller companion galaxy or evidence of a past merger event, given the disturbance mentioned above. However, the resolution of the image makes it difficult to ascertain the true nature of the interaction.

The overall color of the galaxy indicates it's a relatively mature system, though with ongoing, though subdued, star formation within the disk.
