The observed galaxy exhibits a disturbed morphology, suggestive of an ongoing or recent interaction or merger event. The primary body appears diffuse, lacking a well-defined spiral structure or prominent bulge.  There are at least two distinct concentrations of light within the galaxy's profile, indicating potentially separate galactic nuclei or regions of intensified star formation triggered by tidal forces. There is a noticeable tidal tail or bridge of luminous material extending outwards, further supporting the hypothesis of a gravitational interaction. The overall color of the galaxy appears relatively redder than typical spiral galaxies, potentially indicating an older stellar population and ongoing elevated star formation.
