The galaxy presents a morphology suggestive of a system undergoing a merger. The primary body of the galaxy appears relatively smooth and somewhat spheroidal, with a dominant yellowish hue, which may indicate an older stellar population. A secondary component, less luminous and bluer in color, is observed in close proximity, potentially interacting or already merging with the larger galaxy. There is evidence of tidal features or distortions, hinted at by the asymmetry and faint extensions emanating from the main bodies. Overall, this galaxy displays characteristics consistent with late-stage galaxy merger.
