This galaxy, at a redshift of approximately 0.207, appears to be an interacting system. The overall morphology suggests a disturbed state, possibly indicative of a merger event. The galaxy exhibits a centrally concentrated luminosity profile, with a slight elongation that suggests the system is not fully relaxed. There is a noticeable extension, which could be the result of tidal interactions. The primary luminous component is relatively smooth in appearance, while other distinct knots of light are present, potentially representing interacting galaxies or regions of enhanced star formation triggered by the interaction. The colour distribution shows a tendency toward redder colours in the central region, with bluer colours potentially more prevalent in the tidal features. This could suggest older stellar populations in the core and younger populations in the outskirts, possibly indicative of ongoing star formation. The galaxy exhibits a moderately high mass. The system is possibly in late stage of a merger. 
