This galaxy exhibits a disturbed morphology, indicative of a possible ongoing or recent merger event. The light distribution appears irregular, with a central, somewhat amorphous, bulge-like structure dominating the core. Faint, diffuse tidal features are visible extending outwards, suggesting gravitational interactions. A color gradient can be observed, with the central region appearing redder in comparison to the outer regions, which show bluer tinges. This suggests the central region is potentially dominated by an older stellar population. Overall, the galaxy's structure deviates significantly from a standard elliptical or spiral morphology.
