This galaxy presents as a spiral galaxy viewed at an angle closer to face-on. The disk structure is evident, exhibiting well-defined spiral arms extending from a central region. The spiral arms display a tightly wound morphology. The galaxy's color profile reveals bluer hues within the spiral arms, indicative of ongoing star formation. The central region appears more yellow, suggesting an older stellar population and a possible bulge component. The galaxy doesn't show obvious signs of significant tidal interactions or major mergers, although some minor irregularities or disturbances might be present in the outer regions of the disk. Dust lanes are apparent within the spiral arms, obscuring some of the background starlight.
