The galaxy appears as a face-on spiral, exhibiting a relatively small, bright central bulge and a disk structure. The spiral arms are present but somewhat flocculent and patchy, hinting at ongoing but perhaps not highly organized star formation within those regions. The disk itself is more elongated than circular. Color gradients suggest a distribution of stellar populations, with bluer hues potentially associated with younger stars within the arms and a slightly redder hue concentrated towards the central bulge. The outer regions of the galaxy are more diffuse and less well-defined, indicating a lower surface brightness. There is a faint hint of a bar feature bisecting the central bulge, as well as some signs of minor tidal disturbances. Overall, the galaxy presents a morphology consistent with a late-type spiral galaxy undergoing moderate levels of star formation.
