The galaxy presents as a merging system, characterized by two distinct, luminous components. Both components exhibit a generally smooth morphology, with no apparent spiral arm structure or prominent dust lanes visible at this resolution. The color indices suggest that stellar populations are likely present. The overall shape of the combined system deviates significantly from a perfect ellipse, indicative of tidal interactions and gravitational disturbances associated with the merger event. The system appears to be at a relatively early stage of the merger process, with the cores of the two progenitor galaxies still discernable as separate entities. There is a subtle asymmetry in the light distribution. The merger appears to be in process.