The galaxy appears to be a spiral galaxy exhibiting a somewhat disturbed morphology. There are hints of a disk structure, although it is not clearly defined. The galaxy has a bright central bulge with moderate star formation activity. The colors suggest a mix of stellar populations, with the bulge potentially containing older, redder stars. The outer regions show hints of younger, bluer stars, which is indicative of ongoing or recent star formation in these areas. There is some evidence of tidal interactions, seen as faint distortions or extensions in the galaxy's overall shape. The galaxy does not appear to be undergoing a major merger, though there seems to be a minor disturbance with a slight asymmetry suggesting recent interaction with a smaller galaxy.