This galaxy exhibits a complex morphology, appearing to be in a state of interaction or merger. The primary body of the galaxy displays a somewhat smooth, centrally concentrated luminosity profile, although it deviates significantly from a perfect elliptical shape.  There are clear signs of disturbance or tidal features. Two distinct luminous components are visible, with one appearing as a bright, slightly bluer core and the other exhibiting a more diffuse, reddish coloration. These components are separated by a region of lower surface brightness, suggesting either tidal stripping or the presence of distinct galactic nuclei. The overall shape of the system is irregular, with extensions or tails visible, indicative of gravitational interactions.  The color gradient across the galaxy suggests variations in stellar populations, with the bluer regions potentially indicating areas of ongoing star formation and the redder regions indicating older stellar populations. The system is neither perfectly round nor highly elongated; it presents an intermediate axis ratio. The irregular morphology and multiple luminous components strongly suggest a system undergoing a merger event.
