The galaxy presents a complex morphology, exhibiting characteristics of both a smooth, elliptical-like structure and features indicative of galactic interaction. The central region displays a relatively smooth profile, but there are clear signs of disturbance and asymmetry in the outer regions. Filamentary structures are present, potentially signifying tidal tails or debris resulting from a past or ongoing merger event. The color gradients within the galaxy are not uniform. Blueish hues concentrated in certain regions may indicate areas of active star formation. Redder areas, particularly toward the central bulge and in some of the disrupted structures, likely signify older stellar populations and/or dust obscuration. The irregular shape suggests a non-equilibrium state, possibly induced by the interaction with another galaxy or gravitational disturbances from the intergalactic medium. This particular galaxy appears to be in a stage of transition or evolution, driven by dynamic interactions and merging processes.
