The galaxy appears to be a spiral galaxy, although its structure is somewhat disturbed. The central bulge is visible and exhibits a yellowish hue, potentially indicating an older stellar population. There is evidence of a disk structure. Faint blue regions are seen, suggesting the presence of younger, hotter stars. The disk does not seem to be a perfectly flat plane. There is a potential merger with another galaxy happening, disturbing the overall structure of the main galaxy. A tail is present in one of the merging galaxies.
