The galaxy appears to be a spiral, viewed at a significant inclination. The central bulge is prominent, exhibiting a yellowish-orange hue, suggestive of an older stellar population. Faint blue regions extend away from the central bulge, which is likely a disk-like structure. The galaxy does not show any obvious signs of major disturbances or interactions with other galaxies. There is no apparent tidal tail or obvious asymmetry that would suggest a recent merger. There is some possibility of a minor interaction, as the shape of the arms are a bit disturbed. The galaxy appears to be actively forming stars, particularly in the outer regions of the disk, which is consistent with the galaxy having a significant mass in stars.
