The galaxy presents as a somewhat amorphous object. There is evidence of a disk-like structure, though it appears relatively disturbed. The central bulge is somewhat prominent, appearing more orange/red in coloration, suggesting an older stellar population. The galaxy appears to have some star formation activity. It is difficult to determine the specific Hubble type due to the irregularities observed, however, based on its apparent disky features, it may be a spiral or lenticular galaxy undergoing some kind of interaction, such as a minor merger. The galaxy's light is slightly more concentrated in its center and decreases in its edges.
