The galaxy presents as a system undergoing a significant interaction or merger event. The primary body of the galaxy appears disturbed, with a non-uniform distribution of light indicative of structural disruption. A prominent central condensation suggests the presence of an active galactic nucleus or a region of intense star formation activity, exhibiting a slightly redder hue compared to other regions. Fainter, diffuse extensions or tidal features are visible, likely resulting from gravitational interactions. The galaxy displays a complex morphology, exhibiting both smooth and irregular components. Its overall shape deviates considerably from a regular elliptical or spiral form. There is evidence of ongoing or recent star formation, particularly in areas exhibiting a bluer color. The overall color indices suggest it is an intermediate redshift galaxy with moderate stellar mass and star formation rate.
