The galaxy presents with a spiral morphology, exhibiting a prominent central bulge that appears approximately circular and exhibits a bright, concentrated luminosity. The bulge color is consistent with an older stellar population. Spiral arms emanate from the central bulge, displaying a somewhat patchy structure. These arms are not uniformly distributed, suggesting possible gravitational interactions or disruptions. The galaxy disk shows a bluish tint, especially in the spiral arms, which indicates the presence of younger stars. The disk appears to be significantly disturbed. There is also an indication of ongoing or recent merger activity or tidal interaction with another galaxy due to morphological distortions.
