The galaxy presents as a relatively smooth and somewhat amorphous object. Its overall color appears bluish, suggesting the presence of a younger stellar population and ongoing star formation. The central region is brighter and more concentrated than the outer edges, indicating a higher density of stars toward the core. Although the galaxy appears largely smooth, subtle irregularities in its shape hint at possible disturbances, such as tidal interactions or past minor mergers. The object exhibits a nearly round morphology, with only a slight deviation from perfect circularity. There is no clear evidence of a prominent disk structure or spiral arms. The galaxy appears to be undergoing some sort of merging process.
