This galaxy appears to be an interacting system, likely in the process of merging. Two distinct components are visible, each showing a concentrated, somewhat elliptical morphology. The upper component is oriented roughly horizontally, while the lower component is slightly tilted relative to the horizontal axis. Both components exhibit a yellowish-white hue, suggestive of an older stellar population, although hints of bluer light, possibly indicating younger stars, are present along the outer edges of the components. There are some visible dust lanes within the galaxy and some signs of tidal tails which are more concentrated along the bottom component, alluding to gravitational disturbances. The overall structure indicates a significant disruption of each galaxy's original morphology, confirming the ongoing interaction.
