The galaxy presents as a relatively small, faint spiral galaxy with a disk oriented somewhat face-on relative to our line of sight. The spiral arms are discernible, though somewhat flocculent and ill-defined. There is evidence of active star formation within the spiral arms, indicated by regions of bluer coloration. The central bulge appears to be relatively small and not particularly prominent. The galaxy does not appear to be perfectly symmetrical; one side shows signs of disruption, possibly due to interaction with another galaxy, though no obvious companion is immediately apparent in this image. The overall structure suggests a late-type spiral galaxy undergoing active star formation within its disk.
