The galaxy presents a moderately disturbed morphology, indicative of ongoing or recent gravitational interactions. The central region appears somewhat smooth and elliptical in shape. A tidal tail extending outwards is also observed, suggesting the remnants of a tidal interaction. The galaxy displays a color gradient, with the central bulge exhibiting a yellow-orange hue, indicative of an older stellar population. Bluer colors are observed in the outer regions, potentially indicating ongoing star formation. The overall form indicates that the galaxy is undergoing significant activity, with a high likelihood of a recent or ongoing merger event. The galaxy presents a moderate redshift, which suggests that the galaxy is relatively distant.
