The galaxy presents as a disturbed system, showing characteristics indicative of a possible merger event. The primary body displays a disrupted morphology, with asymmetry evident in its overall shape. There is an uneven distribution of light across the galactic disk; the center of the disk is more luminous. There seems to be at least one luminous feature extending outwards, suggesting a tidal tail resulting from gravitational interaction. A separate, less prominent component appears connected or in close proximity to the main galaxy body, further supporting the merger hypothesis. The features are not well-defined, indicating a significant degree of disruption within the system.
