The galaxy presents as a face-on spiral structure, exhibiting a distinct disk. The spiral arms are prominent, showing a somewhat flocculent morphology. Evidence of a central bulge is not obvious, with a more diffuse central region. The color profile indicates ongoing star formation, particularly concentrated within the spiral arms, as evidenced by a bluer hue. There also appears to be a recent or ongoing interaction or merger event, indicated by irregularities in the shape of the disk and tidal tails. The overall form is slightly disturbed, lacking a high degree of symmetry. The light from the disk appears more luminous than the central region. There is no evidence of a strong bar structure within this galaxy.
